The galaxy presents a largely smooth, rounded morphology. It exhibits a centrally concentrated luminosity profile, suggestive of an elliptical galaxy. The overall color appears to be redder, indicating an older stellar population. There is evidence of a possible minor interaction or disturbance on the periphery, with what looks like a small smudge to the left of the bright center. The central region is relatively featureless, lacking prominent spiral arms or dust lanes. The galaxy's apparent regularity and color suggests a relatively quiescent state, with low ongoing star formation.
