The galaxy presents a morphology suggestive of an ongoing merger or strong tidal interaction. Two distinct luminosity concentrations are visible. The larger, more prominent component exhibits a relatively smooth, centrally concentrated light profile, appearing roughly elliptical. Its color is biased towards the blue end of the spectrum. The smaller, secondary component shows a more diffuse and disturbed morphology. It is yellower in color, indicating potentially older stellar populations or higher dust content. There are faint hints of tidal tails or bridges extending between the two components, which further supports the interaction hypothesis. Overall, the system shows signs of low-level star formation activity.
