The galaxy presents as a centrally concentrated, relatively smooth structure. Its overall morphology suggests a system dominated by a spheroid, with a high degree of central light concentration. The color appears generally redder, indicative of an older stellar population and lower levels of ongoing star formation. There's little evidence of prominent spiral arms or dust lanes. The galaxy appears relatively undisturbed, with no clear signs of recent or ongoing major mergers or significant tidal interactions. A slight asymmetry in the outer isophotes may hint at minor disturbances, but the dominant impression is that of a relaxed system. Overall the galaxy can be characterized as an elliptical galaxy. 
