The galaxy presents as a spiral type, though the spiral arms are not particularly well-defined or tightly wound. The disk structure is quite prominent and viewed at an oblique angle. The central bulge appears relatively small and not overly luminous compared to the disk, but it does exhibit a concentrated luminosity. Patches of brighter, bluer regions are visible throughout the disk, suggestive of active star formation. There is a slight indication of a bar structure in the center. The overall color profile suggests a mix of stellar populations, with both older, redder stars and younger, bluer stars contributing to the integrated light. The galaxy appears relatively undisturbed with no major signs of interaction, although there might be minor disturbances in the disk that could indicate a past minor merger.
