The galaxy appears as a flattened, elliptical structure, with a major axis significantly larger than its minor axis. It exhibits a yellowish hue, suggesting an older stellar population dominating its composition. There is a smooth appearance, lacking distinct spiral arms or prominent dust lanes. A slight central concentration is present, indicating the possible presence of a bulge or core region. No signs of significant ongoing star formation are readily apparent in the visual bands. There is no evidence of tidal tails, mergers, or strong gravitational distortions in the immediate vicinity, suggesting it is a relatively undisturbed system.
