The galaxy presents as a relatively smooth object with a distinct elliptical morphology. Its shape is elongated, with an approximate ratio of major to minor axis of around 5:2. The light profile appears centrally concentrated, with the highest intensity observed in the nuclear region. The colour gradient displays a redder hue in the central bulge, transitioning to slightly bluer colours towards the outer regions of the disk. There are very slight irregularities or subtle disturbances in the outer regions, but the overall structure appears largely undisturbed and non-interacting. There is no discernible spiral arm structure or prominent dust lane. Given the redder color and smooth morphology, this galaxy is likely to be composed mostly of older stellar populations. 
