The galaxy presents as a fairly smooth, elliptical structure with a high degree of central concentration. It appears to be quite rounded. There is a distinct lack of discernible spiral arms or prominent dust lanes. The core region displays a bright, relatively uniform luminosity, suggesting a significant population of older stars or possibly an active galactic nucleus. The outer regions of the galaxy fade gradually into the background sky, with a somewhat diffuse halo. There is no evidence of major ongoing mergers or significant tidal disturbances. Slight asymmetry in the outer envelope suggests minor gravitational interactions may have occurred in the past. The color profile indicates a population of older stars dominating the light output, giving it a slightly redder overall hue.
