The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. The outer regions show a gradual decrease in luminosity, displaying a faint bluish tinge. The overall structure lacks prominent spiral arms or significant dust lanes, indicating it is likely an early-type galaxy possibly an elliptical or lenticular galaxy. There is little evidence of recent major merger activity, though a very slight asymmetry might suggest a minor disturbance. The galaxy appears well-defined without any obvious tidal features extending beyond its main body. The color gradient suggests a radial change in stellar population and/or dust content.
