The galaxy presents as an elongated, cigar-shaped structure, with a major axis visibly exceeding its minor axis. The central region exhibits a concentration of light, suggestive of a bulge component. A smooth, diffuse halo surrounds the central bulge, fading into the background. There is minimal evidence of distinct spiral arms or other prominent features within the disk. The color gradient across the galaxy hints at a possible composition gradient, with the central bulge potentially exhibiting redder hues compared to the bluer disk regions. Star formation activity appears relatively subdued, based on the lack of prominent blue knots or HII regions.
