The galaxy presents as a relatively compact object. Its overall color appears predominantly redder, suggesting an older stellar population or significant dust obscuration. There is a slight indication of some subtle, possibly tidal, features. These features are not well-defined but hint at a past or ongoing gravitational interaction. No distinct spiral arms or a clear disk structure are discernible, which would be expected if this object was undisturbed. The galaxy's light profile appears relatively smooth and centrally concentrated, although not perfectly elliptical, which could result from a recent merger or disturbance.
