The galaxy appears as a centrally concentrated object with a largely smooth morphology. It exhibits a moderate ellipticity, appearing mostly round. The galaxy presents with a predominantly yellow-red hue, suggesting a relatively older stellar population with reduced recent star formation. There is a possible indication of minor tidal disturbance or interaction in the form of a small distortion or asymmetry in its outer isophotes. It appears as though a smaller, nearby companion galaxy may be interacting with the primary object.
