The galaxy presents a largely smooth, elliptical morphology. The color is mostly a yellow-white hue, suggesting an older stellar population with few young, hot stars. There is a central concentration of light towards the nucleus, but no distinct spiral arm structure or prominent dust lanes are visible. The overall appearance is indicative of a relatively evolved system with a suppressed rate of star formation. There is evidence of a possible interaction with a nearby galaxy. The galaxy displays a mostly round profile. Any signs of merger are minor, but there is some disturbance of it's mostly round shape.