The galaxy presents as a moderately luminous, somewhat elliptical structure. Its color gradients suggest a population of older stars, particularly toward the central bulge, which exhibits a yellowish hue. The outer regions appear bluer, indicative of ongoing, albeit subdued, star formation activity. The galaxy displays a generally smooth morphology with no readily apparent spiral arms or strong tidal features. There are hints of minor disturbances in the disk, but on the whole the galaxy appears relatively relaxed and unperturbed. It is classified as an intermediate system between round and elongated, with a high probability of non-merging status. Overall, the galaxy appears to be a massive system transitioning from active star formation to a more quiescent state.
