The galaxy appears as a slightly elongated, diffuse object. Its overall color is bluish-white, possibly indicating a population of younger, hotter stars, though the color is not intense. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or other distinct features. It exhibits a somewhat cigar-like shape, not perfectly round. There are hints of possible tidal disturbances or minor interactions, although the galaxy generally maintains a coherent structure. There is no obvious central bulge. Given these properties, this could be a low-mass, star-forming galaxy, possibly undergoing some minor gravitational interaction. It does not look like it is undergoing a significant merger.