The galaxy appears to be undergoing a significant interaction, possibly a merger. It exhibits a disturbed morphology, with two distinct luminous components. One component presents a yellowish-orange hue, suggestive of an older stellar population. The second component shows a bluish color, which indicates the presence of younger, hotter stars and potentially ongoing star formation. The galaxy's overall shape is irregular and elongated, lacking a clearly defined spiral or elliptical structure. There is an indication of tidal features or distorted arms connecting the two components. The concentration of light appears to be moderate. Based on the observed color and morphology, the system appears to be in an intermediate stage of merging.
