The galaxy presents a largely smooth and featureless morphology. It appears to be primarily spheroidal in shape, exhibiting a centrally concentrated luminosity profile that gradually fades towards the outer edges. There is a subtle color gradient visible, with the core region appearing slightly yellower, suggesting a population of older stars dominating the central region. The outer regions exhibit a hint of bluer hues, potentially indicating a small amount of ongoing or recent star formation. There is no prominent disk structure visible, nor are there any obvious signs of tidal disturbances or ongoing mergers. The galaxy appears relatively isolated and relaxed in its morphology.
