The galaxy exhibits a disturbed morphology, potentially indicative of a merger event. There are signs of a central bulge, with indications of two distinct cores present, one possibly more pronounced in the redder wavelengths. The overall color profile suggests intermediate to evolved stellar populations are dominant with hints of ongoing, but localized, star formation. The galaxy appears to be transitioning toward a more spheroidal shape, possibly as a result of the gravitational interactions. The luminous material is relatively diffuse, suggesting a significant amount of older stars.&#x20;
