The galaxy presents as a single, dominant, centrally concentrated structure. It exhibits a relatively smooth, diffuse morphology, lacking prominent spiral arms or distinct features indicative of active star formation in a disk. The galaxy's overall shape approximates an ellipse, showing a slight deviation from perfect circularity. The light distribution appears concentrated towards the core, diminishing in intensity with increasing radial distance. The central region has a yellow color, and the rest of the galaxy is more white. There is no clear dust lane. The overall shape and smooth appearance suggest the galaxy may be of an elliptical or lenticular type. No clear signs of a major merger event are apparent, although a possible, subtle perturbation in the outer envelope might be present. Overall, the galaxy appears to be a fairly mature, quiescent system.
