The galaxy presents as a spiral type with a discernible disk structure. The disk exhibits relatively tightly wound spiral arms, though the resolution limits precise arm characterization. Two spiral arms appear to dominate. The galaxy displays a moderate central bulge, yellowish in hue, which likely indicates an older stellar population concentrated towards the center. Star formation appears to be ongoing, visible as bluer regions within the spiral arms. There's no evidence of a major merger or significant tidal disturbances affecting the overall morphology. The disk appears to be viewed at a moderate inclination. There is a possible weak bar feature noted in the central region.
