The galaxy presents a distinct, elongated morphology, consistent with a disc-shaped structure viewed at a high inclination. There is a central bulge that appears relatively smooth and concentrated. The color gradient transitions from a reddish hue in the central bulge to a bluer tone in the outer regions of the galactic disc. This color difference suggests a stellar population gradient, with older, redder stars dominating the bulge and younger, bluer stars populating the disc. The disc itself exhibits a somewhat diffuse texture, lacking sharply defined spiral arms. The outer edges of the galaxy fade gradually, indicating a decreasing stellar density with distance from the center. There are suggestions of some minor disturbances in the disk, suggesting a possible interaction of some kind, but the galaxy is not dramatically disrupted.
