This galaxy appears to be a relatively smooth, elliptical galaxy with a moderate degree of central concentration. There is no apparent spiral structure, strong dust lanes, or evidence of ongoing major mergers. The overall color is generally yellowish-red, suggesting a population dominated by older stars and a low rate of current star formation. The galaxy appears roughly spheroidal with moderate ellipticity. There is some indication of minor disturbances in the form of very faint asymmetry, suggesting potential past interactions or minor mergers. The core is very bright and is surrounded by a diffuse halo. 
