The galaxy presents as a somewhat rounded, centrally concentrated object. A prominent bulge is discernible, exhibiting a yellowish hue, suggesting an older stellar population within the core. Surrounding the bulge is a fainter, bluer halo. This outer region likely contains younger, hotter stars. A faint disk component may be present, though its morphology is not clearly defined. No apparent spiral arm structure is evident. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal disruptions, although a minor disturbance is possible. The overall color suggests ongoing, but not extremely vigorous, star formation.
