The galaxy presents as a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The core is bright and yellowish, suggesting a population of older stars. The overall shape appears to be more in between round and elliptical, with a slight elongation evident. There's no clear indication of strong spiral arms or active star-forming regions in the disk based on color. There do not appear to be any major merger events or strong tidal disturbance occuring. There are hints of bluer components, possibly some degree of ongoing, low level star formation, especially in the outer regions of the galaxy. 
