The galaxy presents as a somewhat elongated, though largely smooth, elliptical form. A bright central bulge dominates the structure, exhibiting a yellowish-white hue suggestive of an older stellar population. Surrounding the central bulge is a fainter, more diffuse halo that extends outwards, displaying a subtle blue tint on its edges, which may indicate regions of more recent, though not necessarily vigorous, star formation. There is a hint of a possible tidal disturbance or interaction, perhaps a minor disturbance or extended plume of stars, visible at the periphery, but this is not conclusive. The galaxy appears relatively isolated within the field of view, showing no signs of major ongoing mergers or significant tidal interactions with other large companions. 
