The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology. The central bulge is prominent and appears relatively concentrated and reddish in hue, suggestive of an older stellar population. The overall shape is largely spheroidal, although there's a slight elongation visible. There is a subtle disk structure noted by the slight flattening, but lacks any clear spiral arm structures. The faint bluish outer regions are suggestive of some ongoing, although likely low-level, star formation. There does not appear to be any evidence of major tidal disturbances or ongoing mergers. There are subtle signs of disturbance or gravitational interactions, which could suggest a minor merger is present.
