The galaxy exhibits a smooth, elliptical morphology. It appears somewhat elongated, with a measured axial ratio indicating a moderate degree of flattening. The light distribution is concentrated towards the center, displaying a prominent bulge. The color profile suggests a slightly redder core, potentially indicating an older stellar population in the central region. The overall visual impression is consistent with a relatively evolved system. There is no obvious presence of spiral arms or any sign of recent major mergers or strong tidal disturbances, giving the appearance of a relaxed and undisturbed system.