The galaxy presents as a relatively smooth, elliptical-like system. The light distribution appears centrally concentrated, with a gradual decrease in intensity outwards, suggesting a bulge-dominated morphology. There may be some minor disturbances visible, the galaxy does have a faint arm-like formation to the right of the center. It is slightly elongated in shape. The color indices suggest a population of older stars, as indicated by the redder hue, but there are hints of bluer light suggesting some ongoing, but possibly low-level, star formation. The galaxy appears to be relatively isolated.
