The galaxy presents a predominantly smooth, rounded morphology. It exhibits a concentrated central bulge, characterized by a yellowish-white hue, indicative of an older stellar population. Surrounding the bulge is a more diffuse halo, displaying a slight greenish tint that may suggest ongoing or recent star formation. The overall structure appears relatively undisturbed, lacking prominent spiral arms or tidal features suggestive of major mergers. Minor asymmetries or irregularities are not readily apparent at this resolution. The galaxy's light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions.
