The galaxy presents an elongated morphology, appearing as a somewhat irregular structure. There is evidence of a disk component with a hint of spiral arms and a central bulge. The disk exhibits a moderate amount of patchy star formation with regions of bluish-white emission, suggesting the presence of young, hot stars in these areas. The color gradient across the galaxy indicates a possible transition from younger, bluer stellar populations to older, redder ones.

The overall appearance suggests a galaxy undergoing interactions. There appears to be some distortion in its shape, with an asymmetry that is consistent with a possible tidal disturbance. There is also an indication of a possible tail extending from the galaxy, suggesting ongoing or past gravitational interactions. The galaxy is not perfectly smooth; it has some features and irregularities that suggest it is actively forming stars and likely undergoing mergers.