The galaxy presents as a relatively compact, though not entirely smooth, system. It exhibits a prominent central bulge, appearing yellowish, which suggests an older stellar population. A faint, extended disk surrounds the bulge. This disk demonstrates subtle, yet discernible, features that are more blue in coloration. These features possibly indicate areas of more recent or ongoing star formation. The overall shape indicates the galaxy is primarily disk-like and not particularly disturbed, however the data shows some minor features or disturbances may be present. The galaxy does not appear to be undergoing a major merger. Based on the color gradients, the galaxy seems to be in a transitional state, possibly between a more passive and a star-forming phase.
