The galaxy presents as a relatively smooth and rounded structure, with a dominant central bulge exhibiting a yellowish-orange hue. This central region appears to be actively undergoing a merger with a smaller, secondary body of similar color and brightness. The overall light distribution suggests a centrally concentrated mass, with minimal evidence of a disk component. The lack of spiral arm structure or prominent dust lanes further supports the classification as a possible elliptical or lenticular galaxy experiencing a minor interaction. The system's color indicates an older stellar population, implying a lower ongoing star formation rate. Faint, diffuse extensions may hint at tidal features resulting from past gravitational interactions.
