This galaxy presents as a slightly elongated, disk-like structure with a concentrated central bulge that shines with a yellow-white hue, indicating a population of older stars. Fainter, diffuse material extends outwards from the core, suggesting a possible spiral arm structure, although these features are not well-defined. The galaxy exhibits a subtle blue tint around the edges, possibly indicating the presence of younger, hotter stars in the disk. There is some slight distortion or asymmetry in the disk which could be the product of a minor merger or tidal interaction, although the galaxy primarily appears undisturbed. Overall, the galaxy seems to be relatively quiescent.
