The object presents as a relatively compact galaxy, approximately 4 kiloparsecs in radius. It exhibits a generally smooth morphology, with a dominant central bulge that appears somewhat spherical, though subtle deviations from perfect roundness are observed. 

A faint disk component may be present, though it is difficult to resolve details. The color gradient suggests the bulge may contain older stellar populations, appearing redder than the possible disk component, which displays bluer tones indicative of recent star formation.

There may be some disturbance of the galactic structure based on features that appear like tails, possibly suggesting that this galaxy is merging with another.
