The galaxy presents as a centrally concentrated, relatively smooth system. It appears to be elliptical, with a generally round morphology, although there is a slight elongation. The central region displays a higher surface brightness. There are hints of bluer light emission emanating from the central region, potentially indicating recent or ongoing star formation, though the bulk of the galaxy appears to be comprised of older stellar populations, characterized by a redder color profile. There is no evidence of strong tidal features or interactions with other galaxies, though some minor disturbances can't be ruled out. Based on the smooth, symmetrical appearance and color profile, it is likely a massive galaxy with a significant stellar mass.
