The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. The light distribution appears to be relatively even, lacking prominent spiral arms or distinct features. Its overall shape suggests a slightly elongated profile, somewhere between round and cigar-shaped. The galaxy appears to be isolated with no signs of major mergers. It exhibits a noticeable color gradient, transitioning from a brighter, golden-yellow core to a dimmer, redder outer region, suggesting a change in stellar population or dust distribution. Based on its morphology, it is likely to be an elliptical galaxy.
