The observed galaxy presents as a spiral galaxy, viewed at an oblique angle. A distinct central bulge is observed, appearing yellow-white in color. This suggests an older stellar population concentrated in the bulge. Fainter spiral arms extend from the bulge, displaying a bluish hue, indicating the presence of younger, hotter stars. The galaxy appears moderately large, with a clear disk structure. There is a possibility of a weak bar feature across the central bulge. The disk appears relatively smooth, and there are no immediately obvious signs of major ongoing mergers or significant disturbances in the galaxy's morphology. Based on the color gradients and features observed, the galaxy appears to be in a state of moderate star formation activity.
