The galaxy exhibits a morphology that is neither purely smooth nor entirely disc-like, presenting a somewhat amorphous appearance. Its structure is complex, showing evidence of possible interactions or disturbances. There are faint, diffuse extensions emanating from the main body of the galaxy, suggesting tidal interactions or recent merger activity. The primary concentration of light is centrally located and appears somewhat unresolved. Given the apparent disturbances and overall light distribution, the system may be undergoing a merger event or experiencing a period of significant star formation. The color indices suggest the presence of both relatively young, blue stellar populations alongside older, redder populations.
