The galaxy presents an elliptical morphology, appearing generally smooth in structure with a concentrated central bulge. The light distribution suggests a centrally dominant, spheroidal component. There are some indications of possible disturbances or tidal features that could indicate ongoing or past merger activity, presenting as slightly uneven light distribution extending from the main body of the galaxy. The object exhibits color gradients, with the central region appearing more yellow-white, potentially indicating an older stellar population, while the outer regions are slightly bluer, hinting at younger stars or ongoing star formation, though the overall rate of star formation appears relatively low.
