The galaxy appears as a slightly elongated, elliptical structure. It exhibits a smooth, diffuse profile, suggesting an absence of prominent spiral arms or significant dust lanes. The central region displays a concentrated luminosity, indicating a likely bulge component. There's a color gradient visible, transitioning from a bluer hue at the edges to a redder hue at the core, which indicates a population of younger stars in the outer regions and older stars dominating the central bulge. There are hints of minor tidal disturbances or asymmetries, though these are not prominent. The galaxy appears relatively isolated, lacking obvious signs of recent or ongoing major mergers.
