The galaxy presents as a relatively smooth, elliptical structure. Its central region exhibits a bright, concentrated luminosity, suggestive of a significant stellar population and possible active galactic nucleus activity. Moving outward from the core, the light gradually diminishes, forming a diffuse halo. The galaxy appears elongated, more cigar-shaped than circular. The overall color gradient shifts from a yellowish-white core to bluish hues in the outer regions, indicating the presence of both older stellar populations in the center and younger, hotter stars forming in the periphery. No distinct spiral arms or dust lanes are apparent. There is no evidence of major tidal disturbances or ongoing mergers, although subtle asymmetries hint at the possibility of minor gravitational interactions.
