The galaxy appears as a centrally concentrated, relatively smooth structure. Its overall shape is elliptical, with an apparent axis ratio suggesting it is likely an oblate spheroid. The central region exhibits a distinct yellowish-orange hue, indicative of an older stellar population. Progressing outwards from the center, the color profile shifts to a slightly bluer tone, though the overall color remains relatively uniform. There are no prominent spiral arms or distinct dust lanes visible. The outer edges of the galaxy diffuse gradually into the background sky, suggesting a lack of sharp boundaries or recent major star formation events in the periphery. The general morphology is consistent with that of an early-type galaxy, possibly an elliptical or lenticular galaxy. The galaxy shows no obvious signs of major ongoing mergers or significant tidal disturbances. Faint asymmetries might be present but are not definitive from the available image.
