The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that emits a significant amount of light, indicating a high stellar density in that region. The light from the central bulge appears yellowish-orange, which suggests an older stellar population. The galaxy appears to be relatively isolated, with no obvious major interactions occurring, but a small possible disturbance cannot be excluded. The edges of the galaxy appear diffuse and are more elongated than circular. 
