The galaxy appears to be a merging system. The primary galaxy exhibits a generally smooth morphology, tending towards an elliptical shape, though it is difficult to discern fine details at this resolution. There is a secondary component or companion galaxy in close proximity, displaying a redder hue, which may indicate an older stellar population or increased dust obscuration.

The overall color gradient of the primary galaxy suggests a higher concentration of older stars toward the center, with a gradual shift toward bluer colors in the outer regions. This could imply ongoing or recent star formation activity, although the rate appears to be relatively low. Evident distortions and irregularities in the morphology suggest gravitational interaction between the two components, leading to tidal features and potential future merging.
