  Using SDSS-DR7 and NASA/IPAC Extragalactic Database spectroscopic data, we
identify 166 galaxies as members of the Ursa Major cluster with Mr < -13.5 mag.
We morphological classify all galaxies by means of carefully inspecting g-, r-,
i-band colour and monochromatic images. We show that the Ursa Major cluster is
dominated by late-type galaxies, but also contains a significant number of
early- type galaxies, particularly in the dwarf regime. We present further
evidence for the existence of several subgroups in the cluster, consistent with
previous findings. The early-type fraction is found to correlate with the mass
of the subgroup. We also investigate environmental effects by comparing the
properties of the Ursa Major early-type dwarf galaxies to those of the Virgo
cluster. In contrast to the Virgo, the red sequence of the Ursa Major cluster
is only sparsely populated in the optical and ultraviolet colour-magnitude
relations. It also shows a statistically significant gap between -18 < Mr < -17
mag, i.e. the Ursa Major cluster lacks early-type dwarf galaxies at the bright
end of their luminosity function. We discover that the majority of early-type
dwarf galaxies in the Ursa Major cluster have blue cores with hints of recent
or ongoing star formation. We suggest that gravitational tidal interactions can
trigger central blue star forming regions in early-type dwarfs. After that,
star formation would only fade completely when the galaxies experience ram
pressure stripping or harassment, both of which are nearly absent in the Ursa
Major cluster.

Astrophysics of Galaxies