This galaxy appears to be a disk galaxy, viewed at an oblique angle. The morphology suggests a galaxy undergoing interaction or exhibiting internal disturbances. There is a central bulge with a high concentration of older stars, based on its reddish color. The disk component appears mottled, indicating active star formation regions with younger, bluer stars. Faint, diffuse extensions are visible, suggesting tidal features caused by a gravitational interaction. The overall shape deviates from a perfect ellipse. The galaxy has a moderate amount of star formation activity.
