The galaxy presents a generally smooth morphology, indicative of an elliptical or lenticular type. The central region exhibits a concentrated and brighter yellowish hue, which likely corresponds to an older stellar population. Moving outward from the center, there is a subtle transition to a slightly bluer and fainter halo or disk-like structure. The galaxy appears largely undisturbed, lacking obvious signs of major mergers or tidal interactions. However, there is a slight asymmetry observed in the outer regions, suggesting a possible minor interaction or internal dynamics at play. Overall, the galaxy appears as a moderately massive system with ongoing, albeit subdued, star formation activity.
