The galaxy presents as an elongated, disk-like structure, likely a spiral galaxy viewed at a significant inclination. There's a noticeable central bulge that is more yellow, suggesting an older stellar population. Fainter blue hues are visible extending from the bulge into the outer regions, indicating the presence of younger, hotter stars within the disk. The overall structure appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. There is no obvious spiral arm structure that can be distinguished at this resolution, which is consistent with it either being a lenticular galaxy or a high inclination spiral with arms that are difficult to distinguish.
