The galaxy appears to be relatively smooth in structure, with a centrally concentrated, bright core that fades into a more diffuse halo. The overall color is predominantly blue, suggesting a relatively young stellar population or ongoing star formation activity, though this activity appears low. The shape is approximately round, showing a slight deviation from perfect circularity but not extending into a highly elongated or cigar-like form. Indications of tidal disturbances are visible in the outer regions. The presence of more minor and major disturbances can be seen, and there is no indication of a recent or ongoing major merger event. The overall morphology suggests a galaxy that has undergone a merger at some point in the past.
