The galaxy presents a generally smooth, elliptical morphology. The object exhibits a central bulge that is noticeably brighter and more concentrated than its surrounding regions. A faint, diffuse disk appears to extend from the central bulge, displaying a slight elongation that suggests a possible cigar shape. Visual inspection reveals no major disturbances such as tidal tails or obvious signs of an ongoing merger. There is a subtle color gradient moving outwards from the center that suggests the average age of stars declines. Although there is not an easily discernible spiral structure, the outer disk appears to have some faint features.
