The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated bulge with a diffuse halo. The core presents a yellowish hue, potentially indicative of an older stellar population. The outer regions of the galaxy become increasingly faint, gradually blending into the background sky. There is a slight elongation to the galaxy's overall shape, deviating modestly from a perfectly circular morphology. No distinct spiral arms or dust lanes are discernible. There is no obvious evidence of major disturbances or ongoing mergers, such as tidal tails or asymmetrical features, although subtle irregularities in the outer halo cannot be ruled out.
