The galaxy presents as a moderately bright, elliptical-shaped structure. Its central region exhibits a high concentration of light, suggesting a dense stellar population, possibly with an older composition. There is a smooth, gradual decrease in luminosity moving outward from the core toward the galaxy's periphery. The overall color appears somewhat yellowish, indicating a likely lack of significant ongoing star formation. Subtle irregularities in the outer regions may indicate past or minor interaction events. The galaxy appears largely undisturbed with no major signs of ongoing mergers or tidal effects. The roundness is somewhat ambiguous, appearing in between round and elliptical.
