The galaxy presents as a complex, multi-component structure. It appears to be a merging system, characterized by several distinct luminous regions. The primary component is centrally located and exhibits a diffuse, yellowish-white glow, indicative of a population of older stars. 

To the northeast, a bluer, somewhat compact region is observed, suggesting active star formation. There is also a smaller, reddish-orange core visible, likely also consisting of older stars. The morphology of the system is disturbed, with irregular extensions and tidal features potentially indicating gravitational interactions. The overall light profile is not smooth, but rather clumpy and asymmetric, supporting the ongoing merger hypothesis.
