This galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, centrally concentrated light profile, with a lack of apparent spiral arms or prominent dust lanes. The color appears relatively uniform across the galaxy, trending toward redder hues. There is no obvious nucleus or distinct structural features such as bars or rings. Based on its smooth morphology and redder color, this galaxy likely belongs to an older population of stars and has a low rate of star formation. No signs of any major disturbances or recent mergers are apparent. 
