The galaxy presents as an elliptical-type morphology with a smooth, largely featureless appearance. It exhibits a concentrated central bulge region of high luminosity, surrounded by a more diffuse halo extending outwards. The overall color profile suggests an older stellar population, with a dominant yellow-red hue. There is no apparent spiral arm structure or dust lane obscuration visible. The general roundness and lack of significant morphological distortions indicate a galaxy that has not undergone a recent major merger event. It also may not have any current active star formation.
