The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical or possibly a highly inclined disk, with no readily discernible spiral arm structure. The central bulge is prominent and bright, transitioning smoothly into a fainter, more diffuse halo. The color gradient suggests a population of older stars dominating the bulge, with slightly bluer regions extending outwards, potentially indicative of more recent, albeit subdued, star formation activity. Subtle, minor disturbances or irregularities in the outer regions hint at possible past interactions or minor mergers, but no clear, large-scale tidal features are evident. The galaxy's light profile diminishes gradually from the core, implying a fairly relaxed and evolved system.
