The galaxy presents as a single, mostly homogenous object. It is fairly smooth in appearance, with a bright central region that decreases in luminosity gradually towards its edges. The overall shape is elliptical, though it is not perfectly circular, possessing a somewhat elongated form. There is a suggestion of slight disturbances in the outer regions, potentially indicating minor tidal interactions or recent accretion events. Color analysis reveals a predominantly yellow-red hue, indicative of an older stellar population with reduced ongoing star formation.
