The galaxy presents a morphology consistent with an elliptical galaxy or a lenticular galaxy seen at a slight angle. Its overall color appears yellowish-orange, suggesting an older stellar population and a relative lack of ongoing star formation. The galaxy exhibits a smooth, centrally concentrated brightness profile with a well-defined nucleus. There is some evidence of minor tidal disturbances or faint features extending outwards, particularly on the sides, potentially indicating past interactions or mergers with smaller galaxies. The galaxy appears relatively isolated, not showing signs of a major ongoing merger. There might be a faint disk component present, given the slight elongation, but further data would be necessary to confirm.
