The galaxy appears as a centrally concentrated system with a smooth, diffuse light distribution. It exhibits a yellowish-orange hue, suggesting a population of older stars. There is no obvious evidence of spiral arms or a prominent disk structure. The object appears generally round, with only slight deviations from perfect circularity. There is no strong indication of any major ongoing merger activity or significant tidal disturbances. A small number of fainter, bluer objects appear in close proximity to the central galaxy, they are indicative of lower mass galaxies within the same group. Overall, the galaxy appears as a relatively quiescent, massive elliptical galaxy.
