The galaxy presents a largely smooth morphology, lacking the distinct spiral arms or bar structure typically associated with disk galaxies. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the core, gradually decreasing towards the outer edges. The overall shape appears roughly elliptical. There is a color gradient visible, with the central region appearing yellower and redder hues becoming more prominent in the outer regions. No major signs of ongoing or recent mergers are apparent, such as tidal tails or strong asymmetries. There might be minor disturbances. The galaxy is likely a massive system with minimal ongoing star formation.
