The galaxy appears to be a relatively small, elongated system. Its light profile suggests a dominant spheroid component with a smooth, centrally concentrated bulge. There is a noticeable color gradient within the galaxy, with the central bulge appearing more yellow/white, indicating a likely older stellar population. The outer regions of the galaxy appear slightly bluer, suggesting some ongoing or recent star formation, but it does not appear to be widespread. Overall, the galaxy seems to be relatively undisturbed, without any major signs of tidal interactions or recent mergers. The shape is somewhat irregular and cigar-shaped, leaning toward an elliptical morphology, but with a hint of disk.
