The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that is slightly elongated. The light from the galaxy is primarily a smooth gradient, brightest at the core and fading gradually outward to the edges, consistent with an older stellar population. The galaxy is more "in between" on the roundness scale, and slightly resembles a cigar shape. There is very little evidence of prominent spiral arms or dust lanes within the galaxy. There is no clear evidence of any major mergers or disturbances in the structure. The galaxy's color appears as a pale blue, suggesting a relatively low level of ongoing star formation. Overall, the morphology suggests an early-type galaxy with a significant spheroidal component.
