The galaxy presents as an elliptical morphology. There is a concentrated central bulge that appears quite bright, gradually fading toward the edges. The luminosity and smooth gradient suggest an older stellar population, with less ongoing star formation observed from its redder color. The shape is moderately flattened, but the overall structure is relatively undisturbed, exhibiting no significant tidal features or asymmetries indicative of recent major mergers. The galaxy appears as a single, coherent object with no indications of multiple nuclei or separate components. 
