The galaxy presents as an elliptical morphology with a moderate degree of elongation. The core exhibits a high surface brightness and a yellowish hue, suggesting an older stellar population. Moving outward from the core, the color shifts to a bluer tone, indicative of younger stars. Faint features are observed, hinting at the presence of spiral arms or tidal disturbances, but these features are not sharply defined. The overall appearance suggests a galaxy that may be in transition, possibly undergoing interactions with another galaxy, or a later stage spiral galaxy. The galaxy appears to be quite large with a mass estimation that is around 10^10 solar masses. Star formation rate is low.
