The galaxy presents as a centrally concentrated, elliptical morphology with a smooth appearance. Its color is generally yellowish, suggesting an older stellar population. The galaxy exhibits a high degree of rotational symmetry around a bright nucleus. The light tapers off smoothly from the center towards the outer regions. There is a slight flattening of the galaxy, indicating some degree of ellipticity. No distinct spiral arms or dust lanes are discernible. There might be a very faint outer halo surrounding the central region. The galaxy appears isolated without any obvious signs of tidal interaction or ongoing mergers.
