The galaxy presents as an elongated, disk-like structure with a noticeable bulge. There is some indication of spiral arm structure, but this is not well-defined, and the arms appear somewhat flocculent. The central bulge exhibits a smoother, more concentrated light profile, suggesting an older stellar population. The color gradient indicates a bluer hue in the outer regions of the disk, implying ongoing star formation. The redder color toward the central bulge may be indicative of dust extinction or an older, redder stellar population. No significant tidal features or obvious signs of interaction with other galaxies are evident in the immediate vicinity. The galaxy's morphology appears relatively undisturbed.
