The galaxy appears as a relatively smooth, elliptical-like structure with a noticeable central bulge. The light distribution suggests a concentration of older stars in the core, indicated by a yellowish hue, which likely corresponds to a more evolved stellar population. The outer regions of the galaxy display a fainter, more diffuse halo. There appears to be a very subtle hint of some disk-like feature, perhaps a spiral arm, but it is difficult to discern. Overall, the galaxy appears to be relatively isolated and undisturbed, with no clear signs of major merger activity.
