The galaxy presents a moderately bright, elliptical morphology, appearing largely smooth in structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The galaxy appears relatively round. A subtle color gradient is observed, with the central region displaying a slightly yellower hue, potentially indicating an older stellar population or increased dust concentration, while the outer regions show a bluer tint, possibly suggesting younger stars. There is evidence of tidal disturbances, suggesting a merger history. Evident of star formation is weak. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy undergoing some form of evolutionary interaction.
