The galaxy presents as a diffuse, elliptical-like structure. It appears largely featureless, with a smooth distribution of light. There is a slight elongation, though it is mostly round. The central region exhibits a concentration of light, suggesting the presence of a galactic bulge or a dense stellar population. The overall color is a warm hue, indicating an older stellar population and/or a higher abundance of dust, with a possible lower specific star formation rate. There appears to be only a minor disturbance in the galaxy.
