The galaxy appears to be an interacting system, likely in the early stages of a merger. It is composed of what seems to be two distinct components: a larger, relatively smooth and roundish galaxy and a second smaller galaxy that shows a more disturbed morphology and perhaps the presence of a disk-like structure. 

The larger galaxy appears to be relatively spheroid in shape, with a somewhat uniform color gradient indicating an older stellar population and relatively low star formation. There is some indication of dust absorption in the central region. The colors present suggest a mix of older stars, with a lack of intense recent star formation activity.

The smaller companion galaxy appears to show the presence of a more defined disk. The presence of bluer regions suggests on-going star formation. Overall, the companion galaxy has a more disturbed shape, supporting the hypothesis of a merger in progress. Both galaxies are quite compact, but with a low to medium mass.

The overall system exhibits a tidal feature, most notably a faint bridge of material between the two galaxies, which confirms the interaction between them.
