The galaxy presents a roughly elliptical morphology, appearing largely spheroidal in shape. The galaxy's light profile exhibits a generally smooth appearance with no obvious spiral arm structures or significant dust lanes discernible. The central region displays a slightly increased surface brightness, suggesting a concentration of stars or a possible active galactic nucleus, though this cannot be definitively confirmed from the image alone. There is a hint of bluer colors towards the central region, potentially indicative of younger stellar populations or ongoing star formation. Overall, the galaxy appears relatively isolated, with no clear signs of major tidal disturbances or ongoing mergers.
