The galaxy appears to be an elliptical or lenticular type, displaying a relatively smooth and concentrated luminosity profile. The light distribution suggests a spheroidal structure, elongated along one axis, giving it a cigar-like shape. The core region shows a significant concentration of light, appearing yellowish-white, which may indicate an older stellar population. Fainter blue light is observed in the outer regions of the galaxy. This observation may indicate recent star forming regions. No distinct spiral arm structures or prominent dust lanes are discernible within the observable features. The overall appearance is suggestive of a system that is relatively undisturbed, with no immediately obvious signs of major mergers or tidal interactions.
