The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light distribution appears to be dominated by an elliptical component, with a high degree of central concentration and a gradual decrease in surface brightness moving outwards. The galaxy exhibits an overall yellowish hue, suggesting a stellar population that is not dominated by young, blue stars, and little dust obscuration. While it is mostly smooth, there is a subtle hint of asymmetry or a faint extension on one side, possibly indicating a past or ongoing minor interaction or merger event. The object has a relatively compact size, with a consistent color profile throughout the object. No spiral arm structures are visible. Overall, it has a round appearance, with a small deviation towards a cigar shape. There are no significant signs of recent major merging activity.
