The galaxy presents as a moderately bright, relatively compact object. It appears largely spheroidal with a smooth, diffuse morphology, suggesting it is likely an elliptical galaxy. There is no obvious spiral arm structure or dust lanes visible. There may be some minor perturbation to its generally smooth shape. The core appears slightly brighter and more condensed than the outer regions of the galaxy, with the intensity gradually diminishing outwards. Color gradients are subtle but the core presents with some blue tinges relative to the rest of the galaxy, indicating possible recent star formation. The overall red color suggests an older stellar population dominates. The galaxy appears relatively isolated, without obvious signs of a major ongoing merger.