The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a smooth, homogenous light distribution suggesting an older stellar population with minimal ongoing star formation. The galaxy appears elongated, with a major axis extending roughly northwest to southeast and a seemingly high degree of flattening along its minor axis. The central region displays a brighter, more condensed luminosity profile, possibly indicative of a galactic bulge. There is no discernible spiral arm structure or dust lane activity visible. The overall color is reddish, indicative of an evolved stellar population, although with varying light temperature throughout the galaxy.
