The galaxy presents as a relatively smooth, elliptical or lenticular structure. There is a central bulge that is primarily yellow in color, indicating an older stellar population. The outer regions exhibit a fainter, more diffuse halo with a slight reddish tint, possibly due to dust obscuration and a mix of older stars. The overall shape is somewhat elongated, leaning toward an 'in-between' shape rather than being perfectly round. No prominent spiral arms or distinct features are visible, suggesting a lack of significant ongoing star formation. There is no visual evidence of any major merger events or tidal disturbances. The morphology is generally quiescent.
