The galaxy presents a largely smooth morphology, exhibiting a centrally concentrated luminosity profile. The galaxy appears roughly circular. The central region displays a yellowish-orange hue, suggestive of an older stellar population. There are hints of a faint, diffuse halo surrounding the central concentration with some blue-ish tinge, potentially indicating the presence of a small population of younger stars. No distinct spiral arm structures or significant dust lanes are discernible in this image. Overall, the galaxy's appearance is consistent with that of an elliptical galaxy, possibly with ongoing, but low, star formation. There are no obvious signs of major mergers or tidal disturbances affecting the galaxy’s structure.
