The galaxy exhibits a morphology that appears to be somewhere in between smooth and disk-like. Its central region is a bright, smooth bulge, surrounded by a fainter, slightly elongated disk component. There seems to be minor disturbances in its spiral arm structure. The galaxy displays a moderate amount of star formation activity, showing areas of bluer light alongside older stellar populations emitting redder light. The light distribution suggests that the galaxy's structure is neither perfectly spherical nor highly flattened, appearing rather like a spiral galaxy but with a dominant bulge. There may be some evidence of possible past interactions.
