The galaxy presents as a somewhat elongated, cigar-shaped structure. It appears to exhibit a smooth morphology, with no immediately discernible spiral arms or prominent dust lanes. The color profile suggests a population of older stars, evidenced by its reddish hue. There is no obvious central bulge, hinting towards a disk-dominated or irregular classification, although the smoothness may indicate it has evolved to a more lenticular state. The lack of strong blue light indicates reduced current star formation activity. No signs of tidal interactions or major mergers are visible in this image. 
