The galaxy presents as a single, relatively smooth, and somewhat centrally concentrated object. It exhibits a slightly elongated shape, appearing more oval than circular. The core region displays a bright, diffuse glow, suggesting a concentration of older stars. A faint, extended halo surrounds the central region, gradually fading into the background. There is little discernible structure, such as spiral arms or dust lanes, implying a morphology tending toward elliptical. Minor, barely visible disturbances, such as faint tidal tails, might be present, indicating a potential history of past interactions or mergers, although the data strongly suggests that a merger is unlikely. The color profile appears primarily reddish, suggestive of an older stellar population with a relatively low star formation rate.
