The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be fairly round in shape with a slight elongation. The light distribution suggests a centrally concentrated bulge, indicated by the brighter, more yellow hue towards the center of the galaxy. The outer regions exhibit a gradual decline in luminosity, with a hint of bluer colors in the disc, hinting at some on-going star formation. There may be evidence of minor gravitational disturbance with a companion galaxy but it is likely not undergoing a major merger event.
