The galaxy appears to be an early-type system, most likely an elliptical. It exhibits a smooth, centrally concentrated luminosity profile with no apparent spiral arm structure. The core is bright and concentrated, and the outer regions gradually fade into the background sky. There is a slight elongation visible. The galaxy's color appears relatively red, indicative of an older stellar population. There may be some evidence of minor disturbances or asymmetries, but it's not quite clear.
