This galaxy presents as a disturbed system, potentially undergoing a merger or exhibiting tidal interactions. Two distinct luminous components are observed. The primary component is a relatively smooth, centrally concentrated spheroid, appearing yellow-white in color, suggesting an older stellar population. Below and slightly offset from the primary spheroid, a bluer, less defined region is present. This bluer region indicates the presence of younger, hotter stars, likely associated with ongoing or recent star formation. Faint tidal features appear to extend outwards from the bluer region, suggesting a gravitational interaction. Overall, the galaxy exhibits a complex morphology indicative of an ongoing evolutionary process.
