The galaxy presents a generally smooth, elliptical morphology. There is a concentrated central bulge that transitions into a less defined, extended halo. The color gradient shows a shift from a yellowish core to a reddish outer region, suggesting an older stellar population throughout the galaxy. The smooth structure, absence of well-defined spiral arms, and the color profile indicate this is a passively evolving galaxy. Evident is a very slight disturbance on the right side of the galaxy, suggesting a very minor interaction with another galaxy. 
