The galaxy appears to be a spiral galaxy seen at an oblique angle, possibly approaching edge-on. A distinct bulge is visible, indicating a spheroidal component, and a faint, extended disk surrounds this bulge. There is a suggestion of possible spiral arm structure in the disk. The light distribution across the galaxy appears uneven and there is some indication of possible asymmetries in the outer regions.

The central bulge exhibits a redder color compared to the outer disk, possibly indicating an older stellar population. Patches of bluer light are observed within the disk, suggestive of younger, hotter stars and active star formation regions. There is some evidence of possible tidal features, which could indicate ongoing or recent gravitational interactions.