The galaxy appears as a relatively compact object with a smooth, elliptical morphology. There is a distinct central bulge that dominates the light profile. The galaxy exhibits a yellowish-orange color, suggesting an older stellar population and a lack of significant ongoing star formation. A slight elongation is observed, with the galaxy appearing more "in between" round and cigar shaped. There is little evidence of spiral arm structure or prominent dust lanes. No obvious signs of major mergers or significant tidal disturbances are apparent, although some minor irregularities cannot be ruled out at this resolution. The overall appearance indicates a passively evolving galaxy with minimal current star formation activity.
