The galaxy presents as a relatively smooth and concentrated structure. It appears elliptical in shape, with a slight elongation. The light distribution is centrally concentrated with a gradual decrease in intensity towards the outer regions. There is no obvious disk component, spiral arm structure, or bar visible. The galaxy appears to be generally featureless, without prominent dust lanes or bright star-forming regions. There is a very slight visual disturbance to the galaxy's morphology, but no clearly defined signs of ongoing or recent major merger activity. The galaxy has a moderate degree of roundness, and no sharp edges.
