The galaxy presents as a relatively smooth, lenticular-like structure with a notable central bulge. It appears quite rounded in shape and it is generally undisturbed. A faint, but noticeable, dust lane bisects the galaxy along its major axis. The light distribution suggests a higher concentration of older stellar populations, particularly within the central bulge region, which exhibits a yellow-orange hue. Star formation is occurring, but at a lower rate. The overall mass is substantial, indicative of a mature system that is not currently undergoing any major merger events, though minor disturbances cannot be ruled out.
