The galaxy appears to be a spiral galaxy, viewed at an inclined angle, close to edge-on. A prominent central bulge is evident, with a moderate size relative to the disk. The disk shows some indication of spiral arm structure, though not strongly defined, with some patchy regions of brighter intensity within the disk. The bulge exhibits a yellow-white hue, potentially indicating an older stellar population. The disk presents a bluer color compared to the bulge, which implies ongoing star formation. No strong bar structure is immediately discernible. The overall morphology suggests a relatively undisturbed galaxy, without evidence of major mergers or tidal disruptions.
