The galaxy presents a distinct spiral morphology. Two well-defined spiral arms emanate from the central region. These arms appear moderately wound, tracing a path outwards from the core. The central bulge is of moderate size relative to the overall disk. A bar structure is present, spanning approximately half the length of the galactic disk. The disk itself appears relatively flat and is viewed nearly face-on. There is no evidence of a major merger event. Subtle disturbances are present within the spiral arms, suggestive of minor interactions or internal dynamics. Star formation activity is occurring within the arms, indicated by the presence of localized bright knots.
