The galaxy presents as an elliptical-like morphology with a centrally concentrated, bright nucleus that appears yellowish-white in color. A smooth, extended halo surrounds the central region, gradually fading into the background sky. No distinct spiral arms or prominent dust lanes are visible. The overall structure suggests a relatively smooth, evolved stellar population with minimal ongoing star formation. Faint bluish hints may indicate the presence of some younger stars, though these are not prominent features. The shape appears approximately in between round and elliptical. There are no visible signs of major disturbances or ongoing mergers; however, there may be a very slight minor disturbance.
