The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a generally yellowish hue, indicative of an older stellar population. A subtle, redder region extending outwards is visible near the top end of the galaxy. This may indicate the presence of dust lanes or ongoing, but relatively low levels of star formation within the galaxy. The overall structure appears relatively undisturbed, with no clear signs of major ongoing mergers. It appears to be an elliptical galaxy. 
