This galaxy exhibits characteristics of a spiral galaxy, albeit somewhat disturbed. The galaxy presents a bright, yellowish central bulge, indicative of a substantial population of older stars. Extending outwards from the bulge, there's a discernible disk structure, but it does not appear as a well-defined spiral. Hints of blue star formation regions can be observed, indicating ongoing star formation. The morphological appearance suggests a mild gravitational interaction, potentially a minor disturbance or a past merger event. Overall, the galaxy appears to have a considerable stellar mass and moderate star formation activity.
