The galaxy appears as a relatively smooth, centrally concentrated object, likely an elliptical galaxy. It presents a largely featureless morphology, with no obvious spiral arms or distinct substructures visible. There may be very small amounts of star formation occurring within the galaxy. The overall color profile leans slightly toward the redder end of the spectrum, which suggests an older stellar population and a cessation of significant star formation in the past. There is no strong indication of ongoing mergers or major disturbances impacting the galaxy's overall structure. The galaxy is generally round.
