The galaxy exhibits a predominantly smooth morphology, appearing somewhat elliptical in shape. A concentrated central bulge is evident, characterized by intense brightness. Surrounding this bulge, a fainter, more diffuse halo is observable, extending outwards. The color gradient suggests a population of older stars, shifting toward redder wavelengths in the outer regions. There is slight asymmetry of the halo and a faint plume or tidal tail of material extending in a north-westerly direction. There is a suggestion of minor disturbance, potentially indicative of a past or ongoing interaction. The overall structure suggests a system approaching quiescence after possibly undergoing a merger event.
