The galaxy presents as a single, largely homogenous object with a smooth, elliptical morphology. The central region exhibits a concentrated brightness, fading gradually outwards to the edges. The galaxy appears generally rounded in shape. The color is predominantly yellow to orange, suggesting an older stellar population. There is no discernible disk structure or spiral arm features. No obvious signs of active star formation are present within the galaxy. There are no visual indications of a major merger event, though a minor disturbance cannot be entirely ruled out given the low resolution.
