The galaxy presents as a disturbed system, possibly undergoing a late-stage merger. The morphology is irregular, with a central, brighter region appearing somewhat amorphous. Faint tidal features are tentatively observed extending outward, suggesting gravitational interaction with another galaxy, or recent accretion events. Color gradients are subtle, but a general trend is observed: bluer colors in the central region, trending towards redder hues in the extended outer regions. There is no well-defined disk. The overall light profile shows that the object is centrally concentrated.
