The galaxy presents a moderately smooth morphology, with a slight elongation suggesting a classification between elliptical and early spiral, or possibly a disk galaxy seen at an angle. The color gradient indicates a concentration of older stars towards the galactic center, as evidenced by the yellowish-red hue. A hint of bluer regions suggests some recent, ongoing star formation, possibly within a faint disk component. There also appears to be moderate disturbance within the galaxy. 