This galaxy appears to be a relatively smooth, elliptical or lenticular system. There is a central bulge that exhibits a yellowish-red hue, which may indicate an older stellar population or a higher concentration of dust. The main body of the galaxy displays a gradual falloff in luminosity from the center outwards. The overall color gradient suggests a transition from older stars in the core to possibly younger stars in the outer regions. There is no evidence of strong spiral arm structure or prominent dust lanes. It appears to be a relatively isolated galaxy without any significant tidal distortions or nearby interacting companions. The lack of any strong blue color indicates relatively little ongoing star formation.
