The galaxy appears to be a relatively smooth, elliptical galaxy with a subtle central bulge. Its color profile suggests a population of older stars, exhibiting a yellowish hue in the core region. The outer regions display hints of a bluer stellar population, though the overall color suggests that star formation is likely subdued within the galaxy. The galaxy's shape is somewhat elongated, appearing nearly round without any clear spiral arm structure. The outer edges of the galaxy fade gradually into the background sky, indicating a diffuse halo of stars. There is no apparent evidence of tidal tails or other signs of recent major mergers or interactions. There seems to be a very slight distortion in the galaxy's shape.
