The galaxy presents a smooth, centrally concentrated morphology. The light profile appears diffuse with no readily discernible spiral arms or bar structure. It exhibits a generally elliptical shape, though some irregularity is noted. The color is relatively uniform, showing a moderate concentration of blue-green light in the core, suggesting some ongoing star formation, though likely at a low rate. Overall the galaxy appears to be a relatively undisturbed system. There is little evidence of a major ongoing merger. There may be some minor disturbance to the outskirts of the system, but more data would be needed to confirm.
