The galaxy presents an elliptical morphology, appearing as a smooth, concentrated structure with a high degree of central light concentration. The galaxy exhibits an oblong shape, suggestive of a system with a significant spheroidal component and potentially some degree of intrinsic ellipticity. There is little indication of prominent spiral arms or substantial dust lanes. The color appears moderately red, potentially indicating an older stellar population and a low rate of ongoing star formation. Subtle visual disturbances are present, hinting at a possible minor interaction or merger event in its past. These disturbances are primarily visible as faint asymmetries in the outer regions of the galaxy's halo. 
