The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated luminosity profile with a gradual decrease in brightness towards its outer regions. The overall shape is largely round. There is a subtle color gradient, with the core appearing slightly redder and the outer regions showing hints of bluer light. These colors suggest a population of older stars in the central region, while the outer regions may contain younger, hotter stars. The galaxy shows no obvious signs of major mergers or significant tidal disturbances, though there are some hints of asymmetry that could point to minor interactions or internal processes. The color and morphology suggest that the galaxy is moderately massive.
