The galaxy appears to be a spiral galaxy with a fairly compact morphology. A bright central bulge is visible, surrounded by a flattened disk. Evidence of spiral arms can be seen, though they are not sharply defined. The galaxy exhibits a blue hue, particularly in the disk region, which suggests the presence of relatively young, hot stars and ongoing star formation. There may be some evidence of tidal disturbances or interactions. The overall structure indicates this galaxy is in an intermediate stage of morphological evolution.
