The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. A slight flattening is observed, suggesting it is not perfectly spherical. There is a hint of a disk structure within the galaxy, but it is not prominent. The galaxy's color profile indicates a population of older stars, which appear with an orange-red hue, particularly in the central bulge. Faint traces of bluer regions are visible in the outer disk, indicative of some ongoing star formation, albeit at a lower rate. The galaxy does not display any obvious signs of major mergers or significant tidal disturbances, but some minor asymmetry is present. Overall, the galaxy appears to be a relatively evolved system with a dominant spheroidal component and subdued star formation activity.
