The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated central bulge. There is little evidence of spiral arm structure or significant star formation regions. The galaxy's color suggests an older stellar population with a higher proportion of redder stars. The overall morphology suggests a relaxed, evolved system. There may be a slight asymmetry, possibly indicative of a past minor merger event, but this is not prominent. There is no obvious dust lane visible. The light appears relatively uniform across the galaxy, with a smooth gradient from the central bulge to the outer regions. The galaxy is a moderate size compared to other objects within the field.