The galaxy appears to be an elliptical type, exhibiting a generally smooth and diffuse light distribution. There is a centrally concentrated bulge with a slightly elongated shape. The overall color is relatively homogenous with a slight reddish-yellow hue, potentially indicating an older stellar population and low levels of dust. There is no strong evidence of spiral arm structure or significant star formation regions within the visible portion of the galaxy. Possible minor disturbance or some minor features are present within the galaxy, but there is no clear evidence of a major merger event. The galaxy appears relatively isolated.
