The galaxy presents as a relatively compact object with a smooth, centrally concentrated light profile. Its color appears subtly redder, suggesting a population of older stars and a low star formation rate. There is a hint of a slightly elongated shape, but without distinct spiral arm structures or a prominent disk. Overall, the morphology indicates a system dominated by a bulge component. There are no clear signs of ongoing major mergers or tidal disturbances, but the possibility of minor interactions cannot be ruled out based solely on this imagery.
