The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. The core region exhibits a significant amount of light, appearing quite luminous compared to the outer regions. The galaxy does not seem to show any significant spiral arm structures or prominent dust lanes. It presents a more spheroidal shape. There appears to be a slight disturbance in its shape, as if it has undergone a minor interaction, but no major merger is readily visible. The galaxy is a reddish-yellow hue, indicating an older stellar population and a potentially low rate of current star formation.
