The galaxy presents as a generally smooth, centrally concentrated object, with a predominantly elliptical morphology. The light profile appears to decline steadily from the core outwards. There is no obvious spiral arm structure or prominent dust lanes discernible in the image. The galaxy exhibits a slight color gradient, transitioning from a somewhat bluer core to redder outskirts, indicating possible variations in stellar populations or dust content with radius. There is no evidence of a significant major merger or tidal disruption. Slight indications show a minor disturbance from galactic interaction but are generally undetectable.
