The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution is largely featureless, lacking prominent spiral arms or a distinct bar structure. It exhibits an approximately elliptical morphology, appearing nearly circular on the plane of the sky. A gradual decrease in surface brightness is observed from the core outwards, with no sharp edges or truncation evident. There is minimal indication of significant tidal disturbances or ongoing merger activity in the immediate vicinity. The galaxy exhibits a green coloration, indicating strong emission in those wavelengths. 
