The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth, diffuse light distribution. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. There is a gradual decrease in luminosity outwards from the core towards the edges of the galaxy. The galaxy's overall shape is somewhat rounded, lacking any significant signs of spiral arms or a prominent disk. Faint, diffuse extensions surround the central body, hinting at a stellar halo. There is a subtle color gradient, with the outer regions appearing slightly redder, potentially indicating a higher concentration of older, cooler stars. There are some minor indications of slight disturbances in the shape of the galaxy, suggesting a possible past merger event.
