The galaxy presents as a moderately bright, elliptical morphology. The galaxy's light is centrally concentrated, exhibiting a smooth, diffuse profile without readily discernible spiral arms or significant dust lanes. The color appears generally yellow-orange, suggesting an older stellar population and a relatively low rate of ongoing star formation. There is a slight elongation, but it is mostly round in shape. No obvious signs of interactions or major disturbances are present, but potentially some evidence of a minor disturbance or merger event.
