The galaxy appears to be in a state of interaction or possible merger. There is a central, somewhat diffuse, structure. The overall morphology is irregular, lacking a clear spiral arm structure. One side of the galaxy exhibits a more prominent extension or tidal tail. This extension is bluer in color compared to the core, potentially indicating a region of active star formation. The main body of the galaxy presents a more yellowish-red hue, suggestive of an older stellar population. There is a visible asymmetry in the light distribution.
