The galaxy presents a predominantly smooth morphology, exhibiting a high degree of central concentration. The overall shape appears approximately elliptical, trending toward round, with only a slight deviation from perfect circularity. There is no discernible spiral structure or bar feature. The light profile suggests a single dominant component. 

Color gradients are subtle. The central region displays a yellowish-white hue, suggestive of an older stellar population. This gradually fades into a bluer periphery, perhaps indicating the presence of some younger stars or a small amount of ongoing star formation in the outer regions. No significant dust lanes or other obscuring features are apparent. There is no obvious indication of any major tidal disturbances or ongoing merger activity. Based on the faint outer regions, it appears to be a massive galaxy with low star formation.
