The galaxy appears to be a relatively smooth, elliptical system, displaying a concentrated central bulge with a gradual decline in luminosity towards its edges. The morphology is predominantly smooth, with little to no evidence of spiral arm structure or significant dust lanes. It displays a slight elongation in shape. The color gradient indicates the core consists of older stellar populations. There is a hint of bluer light in the surrounding area, which may indicate more active, but very modest, star formation. There are no signs of tidal tails or major disturbances, suggesting that this galaxy is not currently undergoing a major merger event.
