The galaxy presents a complex morphological structure indicative of ongoing or recent interaction. The object appears elongated, with a deviation from a purely elliptical shape, suggesting a possible disturbance. There is an irregular morphology present, with indications of tidal features such as faint streams or tails extending from the main galactic body.

The light distribution is not uniform, displaying clumps of higher intensity suggesting active star formation regions. Patches of bluer light are observed, potentially indicative of younger stellar populations, interspersed with regions appearing redder, which could be indicative of older stellar populations or dust extinction.

Based on the overall morphology, the galaxy could be classified as an interacting system or a galaxy undergoing a merger event. Further spectroscopic observations are needed to confirm its composition and kinematic properties.
