The galaxy presents an approximately elliptical morphology. The central region exhibits a high surface brightness, appearing almost unresolved and whitish in color, suggestive of a substantial population of older stars and/or an active galactic nucleus. Moving outward from the center, the galaxy gradually fades into a more diffuse halo. There is a hint of bluer light within this outer region, indicating the presence of younger stellar populations and ongoing star formation, however, this is not a strong feature. Overall, the galaxy appears relatively smooth in texture, lacking prominent spiral arms or significant dust lanes. There may be slight morphological disturbances present, perhaps a possible indication of a minor interaction.
