The galaxy exhibits a morphology suggestive of an ongoing or recent interaction. One component appears as an elongated, yellowish structure, possibly representing a disrupted or tidally distorted disk or spheroidal component. This component shows a smooth texture. The second component presents a more compact, bluish color profile. The galaxy exhibits an overall disturbed morphology, with a tendency towards a cigar shape. The light distribution suggests that the system may be in a state of non-equilibrium. There is no strong evidence of significant tidal tails or extended diffuse emission in the image.
