The galaxy presents as a spiral type, with a generally face-on orientation relative to our line of sight. Prominent spiral arms emanate from a bright central bulge. The arms exhibit a tightly wound morphology. A bar structure is not clearly discernible. The central bulge appears small relative to the overall disk size. Star formation is evident within the spiral arms, as indicated by the patchy blue regions. There are signs of disturbance within the galaxy disk, such as asymmetric distribution of light. The galaxy is generally smooth, with little signs of a recent or ongoing major merger. 