The galaxy appears to be in a state of interaction or merger. There are two distinct luminous components visible. One component appears relatively smooth and more spheroidal in shape, exhibiting a reddish-yellow hue. This may indicate an older stellar population within this region. The second component is more blue, potentially indicative of ongoing or recent star formation. The overall shape is irregular, suggesting gravitational disruption. There also appears to be a very faint arm or tidal tail originating from the lower part of the bluish component. The galaxy presents a disturbed morphology and probable recent merger.
