This galaxy appears to be a spiral galaxy, viewed at a high inclination. It presents a distinct disk-like structure. The central bulge appears prominent and has an orange-yellow hue, suggestive of an older stellar population. Extending outwards from the bulge, we observe faint, diffuse spiral arms. These arms have a bluer tint, indicating the presence of younger, hotter stars and active star formation regions.

The galaxy exhibits signs of tidal disturbances or interactions, seen as asymmetry in the disk and faint extended features.
