The galaxy presents a largely smooth, elliptical morphology. It appears as a well-defined, centrally concentrated spheroid of light. The light distribution is brightest in the center, gradually decreasing towards the edges of the galaxy. The color gradient suggests that the central regions are slightly yellower, perhaps indicating an older stellar population or greater dust obscuration. No distinct spiral arms or bar structures are discernible. There are no obvious signs of major disturbances in the galaxy's structure, such as tidal tails or highly irregular shapes, though there is the possibility of minor disturbances given a slight asymmetry in the outer halo. Overall, the galaxy appears to be a relatively undisturbed system.
