The galaxy presents a predominantly smooth morphology. It appears to be relatively round, exhibiting a shape somewhere between perfectly circular and slightly elliptical. There is no obvious presence of spiral arms or a distinct disk structure. The galaxy appears fairly homogenous, with a centrally concentrated brightness. There are no obvious signs of tidal tails, bridges, or other significant disturbances indicative of an ongoing major merger event, though some minor disturbance cannot be ruled out. The color profile suggests a galaxy dominated by an older stellar population, given the redder hues, but there is also evidence of some blue light, which could be caused by some recent star formation. Overall, it appears to be a relatively undisturbed system.
