The galaxy exhibits a somewhat irregular morphology, possibly indicative of an ongoing or recent merger event. There appear to be multiple distinct luminous regions, suggesting either multiple galactic nuclei or intense star formation regions triggered by tidal interactions. The dominant color of the galaxy is a pale blue, which could be indicative of a moderately high rate of star formation. A region of yellow is observed in a small part of the galaxy, this could suggest the presence of an older stellar population, a region of dust obscuration, or a combination of both. The overall structure is somewhat diffuse, lacking a clear, well-defined spiral or elliptical shape. Given the diffuse and disturbed appearance, further investigation into the galaxy's kinematic properties would be valuable to confirm a possible merger scenario and determine the ages and compositions of the observed luminous regions.
