The galaxy presents as a relatively bright object with a smooth, elliptical morphology. The light distribution is centrally concentrated with a diffuse halo extending outwards. The core region appears a yellow-orange hue. The extended halo appears slightly green. No obvious spiral arm structures or prominent dust lanes are visible. There is no evidence of active galactic nuclei features, such as a bright, point-like source at the core. The galaxy appears isolated, without any obvious signs of ongoing major mergers or tidal interactions with other galaxies in its immediate vicinity, although there may be a minor disturbance. The overall color suggests a mature stellar population with relatively little ongoing star formation.
