The galaxy presents as a somewhat elliptical structure, indicating it is likely an early-type system but with some visible structure. It appears to be a lenticular or spiral galaxy given the disk component. A notable central bulge is present, with a gradual decrease in luminosity extending outwards. One arm is more visible than the other. Its color suggests an older stellar population with minimal ongoing star formation, the galaxy's light profile and colors suggesting a relatively passive system at redshift z=0.092668.
