The galaxy presents as a somewhat elongated structure, with a noticeable central concentration of light. Its overall color appears to be predominantly bluish-white, suggestive of a population of relatively young, hot stars and/or ongoing star formation. The shape of the galaxy is significantly extended, appearing cigar-shaped, with a smoothly distributed light profile. There is no clear evidence of spiral arms or a distinct disk. No major disturbances are apparent in its morphology.
