The galaxy presents as a flattened elliptical or lenticular form, with an apparent major axis roughly twice its minor axis. There is a distinct central bulge that appears bright and concentrated. The bulge exhibits a smooth, featureless profile, suggesting an older stellar population. The disk surrounding the bulge is fainter and appears relatively smooth, with some evidence of subtle spiral arm structures. The colors are slightly bluer on the edges, and distinctly redder toward the center. There are some small visible disturbances in its structure indicating a possible minor merger. Overall, the galaxy exhibits a well-defined structure with some irregularities.
