The galaxy exhibits a disturbed morphology, suggesting an ongoing or recent interaction. The core region appears very bright and centrally concentrated, with some extension along its major axis. A secondary, slightly less luminous condensation is observed close to the core, possibly representing a merging companion or a region of intense star formation triggered by the interaction. Faint tidal features or plumes are visible, extending outwards from the main body of the galaxy, indicating gravitational disruption. The overall color of the galaxy is consistent with an older stellar population, but the bluer color of the secondary condensation may point to areas of active star formation, although this needs to be verified spectroscopically. The system appears to be undergoing a merger based on the disturbed appearance.
