This galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated, diffuse light profile with a gradual decrease in luminosity towards the outer regions. The galaxy is nearly symmetrical and elongated with the light evenly distributed in an ovular shape. There is a hint of blue color in the central region, suggesting the presence of a young star population. There is a dominant, smoothly distributed older stellar population in the galaxy, which is indicated by the overall redder color. There does not appear to be any evidence of significant dust lanes, spiral arms, or other distinct features. The galaxy appears to be relatively isolated, with no immediately obvious signs of tidal interactions or recent mergers.
