The galaxy presents as an elliptical or lenticular type. It exhibits a dominant central bulge, appearing largely smooth and spheroidal. There is a notable concentration of luminosity towards the core, suggesting a high density of stars in that region. The isophotes appear to be generally rounded in shape, though perhaps verging slightly on elliptical. There are no well-defined spiral arms or distinct disk features visible. Faint evidence of a possible minor disturbance or interaction is suggested by subtle asymmetric light distribution in the halo, which might suggest a past merger event or tidal interaction, though this requires further investigation. Its overall color index suggests it is composed of older stellar populations.
