The galaxy presents as a slightly elongated, disk-shaped structure. It exhibits a relatively smooth overall appearance, but with subtle features suggesting internal structure. A brighter, yellowish central bulge is noticeable, surrounded by a bluer disk. The disk appears moderately inclined, with a suggestion of some unevenness or possible arm-like features in the distribution of the bluer light on one side. No obvious signs of a recent major merger are evident, although there might be some indication of minor disturbances in the disk. The color gradient, from the yellower core to the bluer disk, is consistent with ongoing star formation in the outer regions.
