The galaxy presents as a relatively smooth, centrally concentrated object with a subtle disk-like structure. The central bulge is bright and appears roughly spheroidal in shape, exhibiting a yellowish-white hue indicative of an older stellar population. A faint disk component surrounds the bulge, extending outwards and contributing to the overall elliptical appearance of the galaxy. There is some indication of a slight color gradient, with the outer regions appearing marginally bluer than the core, potentially suggesting ongoing or recent star formation in the disk. There does not appear to be any significant signs of tidal disturbances or ongoing merger activity, and the galaxy appears relatively isolated and undisturbed. The overall morphology suggests a relatively evolved galaxy, likely undergoing a period of quiescence in its star formation history.
