The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellow-orange hue suggesting an older stellar population. The galaxy shows a relatively high degree of roundness, with no discernible spiral arm structures or bar features. There is a gradual decline in brightness from the core outwards, with a faint, diffuse halo surrounding the central region. Visual inspection suggests minimal tidal disturbances or signs of recent major mergers.
