This galaxy presents as a spiral with a prominent central bulge. The spiral arms are tightly wound and numerous. The galaxy exhibits a disk-like structure, with a notable inclination relative to our line of sight, resulting in an elliptical appearance. Within the central region, a concentrated, bright area indicates a significant stellar population or active galactic nucleus. The disk is bluer than the central bulge, suggesting ongoing star formation within the spiral arms. There appears to be a weak bar feature spanning across the bulge. There is no evidence of major mergers or significant tidal disturbances and the spiral arms are relatively symmetrical.
