The galaxy presents a generally elliptical morphology, with a high degree of central concentration indicated by a bright, unresolved core. The overall light distribution appears relatively smooth, lacking distinct spiral arm structures. The galaxy exhibits a somewhat rounded shape, with only a slight elongation discernible. A faint, diffuse halo surrounds the central region, gradually fading into the background. There is the presence of some disk-like features, with subtle, low-contrast structures that suggest the possibility of a disk component viewed at a low inclination angle. There is the possibility of a minor interaction or disturbance, potentially in the form of tidal streams or asymmetries in the outer regions, but these are not prominent, and do not suggest an active major merger. The galaxy presents as a quiescent system.
