The galaxy appears to be part of a small group, possibly interacting. One galaxy presents a centrally concentrated, elliptical morphology, with a smooth profile. The color of the central region appears yellowish, suggesting an older stellar population. The other large galaxy in the image is more disk-like in appearance. There is a hint of spiral structure, though it is faint. This disk-like galaxy shows a bluer color, suggesting ongoing star formation. This galaxy may be experiencing a minor gravitational disturbance. The estimated size of the larger galaxy is significant, suggesting a relatively massive system. Overall star formation rates are elevated. The group does not appear to be in a major merger state.
