The galaxy presents as a relatively smooth, centrally concentrated object. The light is generally yellow-white in the central region, possibly indicating an older stellar population. The outer regions display a diffuse, blue-ish hue, suggestive of ongoing star formation. The overall shape appears largely elliptical, with no strong evidence of spiral arms or a prominent disk. There appears to be minor asymmetry in its outer envelope, possibly due to a gravitational interaction. Evidence indicates a relatively low star formation rate. The galaxy exhibits considerable mass, with a possible supermassive black hole powering activity at its core.
