The galaxy exhibits a discernible spiral structure, with moderately wound arms that appear somewhat patchy and fragmented. A prominent central bulge is observed, contributing significantly to the galaxy's overall luminosity. The disk of the galaxy displays a bluish hue, suggesting the presence of younger stellar populations and ongoing star formation. The galaxy shows signs of tidal disruption and possibly a major merger, with distorted morphology and indications of interaction. This suggests that the system may be dynamically young or recently disturbed. Overall color profile indicates active star formation. The galaxy appears to be a spiral galaxy undergoing active star formation and shows morphological signs of a major merger. 
