The galaxy presents as a single, relatively smooth, and rounded object. It appears to have a centrally concentrated light distribution, with the intensity decreasing gradually towards the outer regions. There is no clear evidence of spiral arm structures or a prominent galactic disk. The galaxy exhibits a dominant orange-red hue, suggesting a population of older stars. The overall morphology is suggestive of an elliptical galaxy. There are no signs of major mergers or significant disturbances in the galaxy's structure within the image.
