The galaxy presents a largely smooth, elliptical morphology. There is a concentration of light towards the central region of the galaxy, indicative of a bulge. The light from the galaxy exhibits a color gradient, shifting from a redder hue in the core to a slightly bluer hue at the edges. There is no apparent spiral structure, such as arms or a bar. The galaxy appears relatively isolated, with no obvious signs of major interaction with other galaxies. Faint irregularities in the outer regions may suggest possible minor disturbances, such as a past accretion event or a low-level merger, however the overall structure suggests a more relaxed system.
