The galaxy presents a primarily smooth morphology, with a dominant central bulge. The shape appears to be generally elliptical, trending towards a slightly elongated form. The light distribution suggests a concentration of older stellar populations in the central regions, as indicated by the yellowish hue of the bulge. Fainter, bluer light is observed in the surrounding regions, possibly suggesting the presence of some younger stars or star-forming regions, though these are not sharply defined. There is no readily apparent spiral structure or bar feature. There is no visual indication of a major ongoing merger or significant tidal disturbances. The overall impression is that of a relatively undisturbed, evolved galaxy.
