The galaxy presents as an interacting system, potentially in the late stages of a merger. One component appears to be a relatively smooth elliptical galaxy, exhibiting a concentrated, round morphology with a generally homogenous color profile suggesting an older stellar population. The second component displays a more disturbed structure, with a disk-like morphology. The colors are variable, with redder colors being more prominent, potentially indicating older stellar populations or dust obscuration. There is a strong indication of tidal interaction between the two components with asymmetric morphology, suggesting tidal tails and/or bridges. Overall, the system exhibits a notable disturbance in its morphology. Star formation appears to be subdued.
