The galaxy presents as a relatively smooth, centrally concentrated elliptical or lenticular structure. It exhibits a noticeable elongation, appearing somewhat cigar-shaped in projection. A significant fraction of the galaxy's light is concentrated in a bright, diffuse central bulge. A faint disk component may be present, but it is difficult to distinguish. There's an indication of a minor disturbance or interaction event occurring, possibly in the form of a slight asymmetry or tidal feature. Overall, the galaxy appears to be relatively evolved.
