The galaxy presents as a relatively smooth, disk-like structure. It exhibits a noticeable central bulge that appears yellowish-orange in color, suggesting an older stellar population. The disk component shows hints of spiral arm structure, although they are not sharply defined. The color of the disk appears slightly bluer than the bulge, which could imply the presence of some ongoing star formation. Overall, the galaxy does not appear significantly disturbed, showing no prominent tidal features or signs of a recent major merger. However, a slight asymmetry may be visible in the disk's outer regions.
