The galaxy exhibits an elliptical morphology, appearing as a diffuse, oval-shaped structure. The galaxy's light profile suggests a high degree of central concentration with a smooth, gradually decreasing intensity outwards from the core. The central region is comparatively bright, appearing yellow/white in color, possibly indicating an older stellar population. The outer regions are less defined and fainter, with hints of a bluer hue. No distinct spiral arms or prominent dust lanes are visible. There is a slight asymmetry to the galaxy shape, with a hint of possible minor disturbances. Overall, the galaxy appears relatively undisturbed, with no indications of major ongoing mergers.
