This galaxy appears to be a spiral galaxy viewed at a significant angle to our line of sight, nearing edge-on. The central bulge exhibits a yellowish hue, suggesting an older stellar population. The disk surrounding the bulge is visible as a bluer, more diffuse region, which is indicative of ongoing star formation. The disk is not uniformly bright, with some areas appearing slightly more luminous than others, possibly due to variations in star formation rates or dust obscuration. Overall, the galaxy shows a relatively smooth texture, although some subtle features may be present but are difficult to discern at this resolution. There are no immediately obvious signs of major mergers or strong tidal disturbances, though there may be minor disturbances to its structure. The overall elongated shape is consistent with a disk-dominated system seen at an oblique angle.
