The galaxy appears as a centrally concentrated object with a moderately diffuse halo. The morphology suggests a largely spheroidal structure, exhibiting a mixture of smooth and disk-like features, though the smoothness appears to dominate. Color gradients within the galaxy are subtle, showing a slightly bluer core transitioning to redder outer regions. This indicates a potential population shift from younger, hotter stars in the center towards older, cooler stars in the outskirts. No prominent spiral arms or bars are immediately visible, pointing towards a later-type disk galaxy or an early-type galaxy with some remaining star formation. There may be a minor disturbance due to interactions with other nearby bodies.
