The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a bright, concentrated core region that diffuses outward. There is a gradual decline in surface brightness from the core to the outer edges, suggesting a lack of significant recent star formation activity in the outer regions. The galaxy appears to be slightly elongated in shape, possibly cigar-shaped. There is no evidence of major mergers or significant tidal disturbances. The color appears uniformly yellowish-red. The overall appearance is consistent with a mature galaxy dominated by an older stellar population.
