The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated bulge, with a gradual decrease in luminosity towards its outer regions. There's little evidence of spiral arm structure or significant dust lanes. The overall shape is somewhat round, tending towards elliptical. The color profile suggests a population of older stars, with a bias toward the redder end of the spectrum, particularly within the core, though bluer colors are present. There is no strong evidence of ongoing major mergers or tidal disturbances, though there could be some minor distortions present that are difficult to discern at this resolution. The galaxy exhibits a relatively compact size, appearing small relative to the field of view.
