The galaxy appears to be undergoing a significant interaction, possibly a merger. It presents as an amorphous structure, lacking a well-defined spiral or elliptical shape. There are two distinct bright clumps of luminous matter that are reddish-orange in color. One clump appears larger and more diffuse than the other. Overall, the galaxy is irregular and shows evidence of disturbance, suggestive of gravitational interactions. The galaxy's color indicates an older stellar population. The galaxy appears relatively compact, with an estimated diameter of approximately 5 kpc. Based on its color, disturbed morphology, and relatively compact size, the system is estimated to have a stellar mass of 10^10.5 solar masses, and a star formation rate of less than one solar mass per year.
