The galaxy appears to be a spiral galaxy, exhibiting a generally disk-like structure. The central region displays a noticeable bulge, with an apparent concentration of older stars indicated by a yellowish hue. Extending outward from the bulge are spiral arms. The arms appear somewhat tightly wound. The colour of the spiral arms varies from blue to redder hues, suggesting a mix of stellar populations and ongoing star formation regions. There is no obvious presence of a strong bar structure within the central region. The disk is observed face-on. There are no obvious signs of tidal tails or distortions, indicating that this galaxy is not undergoing a major merger, though minor disturbances cannot be ruled out. Overall, the galaxy seems to be a relatively well-formed spiral galaxy.
