The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in shape, with a slight elongation. The color gradient suggests a fairly evolved stellar population, with the central region exhibiting a more pronounced concentration of older, redder stars. There is no obvious dust lane or spiral arm structure visible, which supports a classification as an elliptical galaxy. The light is generally uniform, with no prominent knots or regions of intense star formation readily apparent in the image. The morphological classification suggests the galaxy is likely not undergoing major mergers or significant tidal disruption, as it appears relatively undisturbed.
