This galaxy presents a somewhat elongated morphology, suggesting a disk galaxy viewed at an oblique angle, not quite edge-on. The central region exhibits a bright, diffuse glow, possibly indicative of a prominent, though not necessarily dominant, bulge or a concentration of stars and gas. Evidence of spiral arm structure is present, albeit not strongly defined. These arms appear somewhat flocculent and loosely wound. Color gradients are observable, with bluer hues concentrated in the outer regions of the disk, possibly signifying regions of active star formation, and a slightly redder tint towards the central bulge. There is a possible bar-like structure spanning across the center of the galaxy. Overall, the galaxy appears relatively undisturbed.
