The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a near-spherical morphology, with no apparent spiral arm structures or significant asymmetries. The core region is noticeably brighter, suggesting a high concentration of stars or an active galactic nucleus. The color profile indicates a potential mix of stellar populations, the central region appears to exhibit somewhat elevated luminosity in g band. There is no apparent signs of ongoing major merging activity, although minor disturbances cannot be ruled out based on the available imaging. The overall appearance suggests a galaxy that is potentially a lenticular or early-type spiral galaxy, based on its smooth appearance and lack of pronounced features.
