The galaxy presents as a spiral type, with a notable disk structure. The disk appears inclined to our line of sight, but not entirely edge-on. Spiral arms are clearly discernible, exhibiting a tightly wound morphology. The central bulge is relatively prominent, displaying a moderate size in relation to the overall disk. The overall color profile indicates the presence of both older stellar populations in the bulge region and bluer, star-forming regions within the spiral arms. A slight asymmetry is observed in the outer regions of the disk, which could be indicative of minor gravitational interactions or disturbances. There is no visible sign of a strong bar structure.
