The galaxy presents as a relatively smooth, elliptical structure with a highly concentrated central bulge. It exhibits a yellowish hue, indicative of an older stellar population, with minimal presence of bluer, younger stars associated with active star formation. The galaxy appears elongated along a principal axis, suggesting a slight flattening of its ellipsoidal shape. There is no visual evidence of spiral arms or a distinct disk structure. The light profile smoothly decreases from the core outwards, which is consistent with a galaxy following a Sersic profile, suggestive of an older stellar population galaxy. There is no visual evidence of a major merger event. Minor disturbances may be present in the outer halo but the resolution is too limited to determine this. The galaxy has a low star formation rate.