The observed galaxy presents an irregular morphology. A bright, concentrated core region is evident, potentially indicative of an active galactic nucleus or a dense stellar population. The galaxy exhibits an asymmetric structure, with a discernible extension or plume emanating from one side of the core. This feature suggests possible tidal interactions or recent merger events, although the overall galactic structure does not appear to be in a late stage merger. The color profile indicates that this galaxy has a higher concentration of blue light. Overall, this appears to be a blue, actively star forming galaxy with a disturbed morphology. 
