The galaxy presents a generally smooth and rounded morphology. The color profile suggests an elliptical or lenticular classification. The central region exhibits a brighter, yellowish hue, possibly indicating an older stellar population. Fainter, reddish regions are present off-center which may suggest some recent star formation. Given the generally smooth appearance and lack of prominent spiral arms or a well-defined disk, it appears to be fairly relaxed, though some minor disturbance or possible merging is present. The galaxy's integrated light suggests a substantial stellar mass and absolute magnitude.
