The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There are no obvious spiral arms or bar structure visible. The galaxy's light profile appears relatively uniform, with a gradual decline in brightness from the core to the outer regions. The central core is bright and concentrated and unresolved, suggesting an older stellar population. The outer regions exhibit a bluer color, which could indicate a more recent episode of star formation. There is no evidence of a major ongoing merger, though there appears to be some minor disturbances in the outer regions.
