The galaxy presents as a slightly elongated, lenticular structure. Its light profile is relatively smooth, with a central concentration of older, yellow stars. There's an indication of a subtle disk component, though the galaxy is largely dominated by its bulge. The galaxy's color suggests a lack of ongoing, intense star formation, consistent with a relatively quiescent stellar population. It exhibits a mild degree of flattening, tending towards a cigar-like shape, but is mostly in between round and cigar-shaped. There is no clear evidence of any major mergers or significant tidal disturbances.
