The object presents as a spiral galaxy, viewed at an oblique angle, but closer to edge-on. There is a prominent central bulge exhibiting a yellowish-white color, suggesting an older stellar population. Fainter spiral arms emanate from the bulge. The spiral arms display a bluer hue, indicative of ongoing star formation. The arms appear somewhat patchy and loosely wound. There is evidence of a weak bar structure crossing the central bulge. Some asymmetry in the spiral arm distribution suggests possible gravitational interaction or past merger event. The overall structure is moderately disturbed but retains recognizable spiral characteristics. 
