The galaxy presents a largely smooth, elliptical morphology. There is a centrally concentrated, bright bulge region that dominates the luminosity profile. The light from the core appears yellowish-white, suggesting an older stellar population. Extending outward from the core is a fainter, more diffuse halo. There is a faint blue tinge at the periphery, suggesting some star forming regions may exist within the disk. The galaxy appears undisturbed, showing no obvious signs of tidal interactions or major mergers. There is no clear dust lane or spiral arm structure visible. Overall, the galaxy seems consistent with an early-type galaxy undergoing relatively little ongoing star formation.
