The galaxy presents a relatively compact morphology. It exhibits a bright central bulge that is approximately circular in projection. Evident in the galaxy's structure are indications of a disk component surrounding the central bulge. The disk appears relatively faint, and there might be some minor tidal disturbances. Based on this image, there might be minor disturbances in the morphology, potentially indicating a past merger event or interaction. There is no evidence of strong spiral arm structure or a prominent bar.
