The galaxy appears to be an elliptical type, characterized by a generally smooth and rounded morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The light distribution suggests a relatively uniform stellar population without prominent spiral arm structures or dust lanes. There is a slight elongation and the galaxy seems to be close to a neighbor galaxy. Overall, the galaxy presents a mature and relaxed appearance, consistent with an early-type classification, exhibiting some interaction with the other nearby galaxy.
