The galaxy presents an overall elliptical morphology. The central region exhibits a bright, concentrated luminosity profile, suggesting a prominent galactic nucleus. Moving outwards from the center, the galaxy displays a gradual decrease in surface brightness, forming a smooth, diffuse halo. The color distribution indicates a slightly redder hue in the central bulge, possibly signifying an older stellar population, while the outer regions exhibit a bluer tint, which might indicate regions of ongoing star formation. There is a slight asymmetry in the outer regions, suggesting the potential for minor gravitational interactions, or perhaps an active galactic nucleus. The galaxy appears relatively undisturbed, with no obvious signs of a major merger event.