The galaxy presents as a somewhat smooth, centrally concentrated object with a slightly elongated, but generally rounded morphology. A dominant, bright central region is observed, surrounded by a more diffuse halo. There appears to be a slight disturbance or merging event occurring, evidenced by a secondary bright spot slightly offset from the primary nucleus. The colour profile suggests the presence of both older stellar populations in the central region, appearing more yellow/white, and possibly ongoing star formation in the outer regions where bluer hues are present. The overall structure indicates a galaxy undergoing some form of interaction, potentially influencing its star formation rate and overall morphology.
