The galaxy presents as a centrally concentrated, smooth object. Its light profile is relatively regular, lacking prominent spiral arms or a distinct bar structure. The color index suggests a galaxy populated primarily by older stars, potentially indicating an elliptical morphology or a spiral galaxy with a prominent bulge and a relatively quiescent disk. There may be little ongoing star formation. The galaxy exhibits a roughly circular shape. There is no obvious evidence of tidal features, strong gravitational lensing, or indications of a recent major merger event. Faint asymmetric extensions might be present, warranting further investigation to ascertain potential minor disturbances.
