The galaxy presents as a moderately luminous elliptical system, displaying a smooth, largely featureless morphology. Its light profile indicates a centrally concentrated spheroid, with the brightest region residing in the core. There is a gradual decrease in luminosity outward from the nucleus, suggesting a relatively old stellar population dominates. Subtle color gradients are observed, with a slightly redder hue towards the center and a bluer tinge toward the outer edges. Overall, the galaxy appears to be relatively isolated and undisturbed.
