The galaxy presents as a distorted spiral or irregular morphology. There is a bright, somewhat diffuse central bulge exhibiting a yellowish hue, suggestive of an older stellar population. Extending from the bulge, at least one discernible arm or tidal feature is present. It appears to be undergoing a period of active star formation, as indicated by the presence of blueish regions within the arm, likely regions of ionized gas and young, hot stars. The overall structure indicates a potential interaction or merger event may have occurred, as the symmetry typically observed in undisturbed spiral galaxies is absent. Redder regions are visible along the arm as well, which also suggest older star populations.
