The galaxy presents as a highly elongated structure, suggestive of an edge-on spiral or lenticular morphology. A prominent central bulge is observed, though its specific stellar population cannot be determined from the image alone. The disk component appears relatively smooth, lacking distinct spiral arm features. The galaxy exhibits a noticeable color gradient, with the central bulge showing a more yellow/orange hue, potentially indicative of older stellar populations. A bluer color is noted towards the edges of the galaxy. Some irregular features are present within the disk, possibly due to dust lanes or recent star formation. The overall shape shows little sign of any major disturbances.
