The galaxy presents as an elongated, cigar-shaped morphology. It exhibits a smooth, diffused light profile, with a central, brighter region suggesting a concentration of stars or potentially an active galactic nucleus, though further spectral analysis would be required to confirm this. The overall color appears reddish-orange, possibly indicative of an older stellar population or significant dust obscuration. There's no clear evidence of spiral arms or distinct features typically associated with actively star-forming galaxies. Minor irregularities may be present, but they're not pronounced enough to definitively categorize the galaxy as undergoing a major merger event. Its estimated size appears to be several kiloparsecs across.
