The galaxy presents an apparent morphology that appears to be a disk galaxy.  The central bulge exhibits a yellow-orange hue, suggestive of an older stellar population, potentially dominated by red giant stars and a lack of ongoing star formation in the core.

A fainter, bluer disk-like structure surrounds the central bulge. The blue color implies the presence of younger, hotter stars, indicating regions of more active star formation within the disk. The features appear somewhat amorphous and disturbed. Faint tidal features are present, suggesting the galaxy has experienced, or is experiencing, a gravitational interaction with another galaxy or has accreted matter.