This galaxy exhibits a spiral morphology, characterized by a prominent central bulge and well-defined spiral arms. The arms appear tightly wound, tracing a clear pattern from the central region outwards. The bulge component appears moderately sized relative to the overall disk, indicating a possible intermediate classification within the spiral galaxy sequence. A bar structure is present, with a notable concentration of stars and gas along its axis. The disk appears relatively undisturbed, with no major signs of ongoing or recent merger activity, though minor disturbances can't be ruled out. Patches of star formation are distributed along the spiral arms, evidenced by regions of enhanced blue emission. The overall color of the galaxy suggests a mix of stellar populations, with the bulge likely dominated by older, redder stars and the disk containing a younger, bluer population associated with recent star formation.
