The galaxy presents as an elongated, cigar-shaped system with a smooth, centrally concentrated light distribution. There is little discernible internal structure, such as spiral arms or prominent dust lanes. The dominant color is a pale yellowish-white, suggestive of an older stellar population, particularly in the central region. Fainter blueish tinges can be observed near the edges, possibly indicative of more recent, albeit subdued, star formation in the outer regions. Overall, the galaxy appears relatively undisturbed, showing no strong evidence of tidal interactions or major merging events. The galaxy exhibits a smooth, elliptical-like morphology.
