The galaxy appears as a single, relatively smooth concentration of light, centrally condensed. It is ellipsoidal in shape, significantly more extended in one direction than the other, with a roundness leaning towards an in-between elliptical form. The overall color profile indicates a dominant yellowish hue in the central region, possibly indicative of an older stellar population. There is a subtle gradient in the radial color profile, shifting towards a slightly bluer or greener color in the outer regions of the galaxy's halo, which may suggest the presence of younger stars or some ongoing star formation. There is no visual evidence of strong tidal features, significant dust lanes, or a prominent spiral structure. There are no indications of a current major merger event.
