The galaxy exhibits an overall yellowish hue, suggesting an older stellar population. The light is centrally concentrated, which suggests a spheroidal morphology. There is a faint, diffuse halo of light extending outwards from the core, possibly comprised of older stars or dust. The disk shows signs of disturbance or features, suggesting a recent or ongoing interaction or merger. The system appears to be actively forming stars. The galaxy is estimated to have a stellar mass around 10^10 solar masses.
