The galaxy appears to be an interacting system, likely in the early stages of a merger. One component presents as a relatively smooth, elliptical-like form with a concentrated core, exhibiting a yellowish-red hue. This suggests an older stellar population.

The second component displays a more elongated and disturbed morphology. There is visible disk-like structure or tidal tail features. This body appears bluer in color, implying the presence of younger, hotter stars and ongoing star formation. The system is compact, with the two components separated by a small distance. Some minor disturbances are visible, and there may be an ongoing merger.
