The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology. It exhibits a concentrated, centrally bright bulge that diminishes gradually with radial distance. Color gradients suggest the presence of older stellar populations dominating the galactic composition, with the central regions appearing more yellow and red, indicative of low levels of current star formation. There is little evidence of spiral arms or dust lanes. The galaxy's shape is generally round, with no obvious signs of major disturbances or ongoing mergers. The overall appearance suggests a gravitationally relaxed system that has largely completed its star formation. The physical size is consistent with an average galaxy.
