The galaxy presents as a tilted spiral structure. A bright, concentrated central bulge dominates the core, surrounded by a moderately inclined disk. The disk exhibits faint spiral arm features emanating from the central region, loosely winding outwards. These arms appear somewhat flocculent. Dust lanes are not clearly apparent, but subtle variations in surface brightness within the disk suggest their presence. The overall color is bluer in the outer disk regions, transitioning to yellower tones towards the central bulge, indicating a likely stellar population difference. The disk is elongated, possessing an elliptical shape.
