The galaxy presents as a dual system, seemingly undergoing an interaction or a merger event. The primary galaxy appears as a slightly elongated structure with a smooth, diffuse light distribution, suggesting a predominantly older stellar population. The central region exhibits a yellowish hue, possibly indicating a concentration of evolved stars.

The secondary galaxy is more compact and displays a bluer color, suggestive of ongoing star formation. Its morphology is less defined, potentially due to tidal disruption from the interaction with the larger primary galaxy. There appears to be a faint bridge of material connecting the two galaxies, further evidence of gravitational interaction. Overall, the system exhibits characteristics consistent with an intermediate stage of galaxy merging, with potential tidal features present.
