This galaxy presents a largely smooth and centrally concentrated morphology. It exhibits a slightly elliptical shape, appearing more elongated than perfectly circular. The color profile indicates a dominant population of older stars, with a yellowish-white hue concentrated in the central bulge region. The outer regions of the galaxy appear slightly bluer, potentially indicating the presence of some younger stars or ongoing star formation, although this activity seems relatively subdued. There is no clear evidence of spiral arm structure or significant dust lanes. The overall appearance suggests a relatively evolved system with a substantial stellar mass. While there might be some minor disturbances evident in the outer regions, the galaxy appears largely undisturbed and does not present a clear merging signature.
