The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, appearing mostly round, with a subtle elongation. No distinct spiral arm structures are discernible. The galaxy exhibits a bright central region, potentially indicating a significant concentration of stars or an active galactic nucleus. Color gradients within the galaxy suggest a mix of stellar populations. The core area appears to exhibit a bluer color, which could indicate younger stars and ongoing star formation, while the outer regions fade into a redder hue. There appear to be no clear signs of a major ongoing merger event, although slight asymmetries and faint outer structures could imply past interactions. The light from the galaxy suggests that it is a relatively large and massive galaxy.