The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated, luminous core that gradually fades into the surrounding galactic halo. The overall color profile indicates a redder hue, suggestive of an older stellar population with a subdued rate of star formation. There are no readily apparent spiral arms or significant dust lanes visible in this image. The galaxy appears largely undisturbed, without obvious signs of ongoing merger activity or tidal interactions.
