The galaxy presents as a singular, relatively smooth object. Its light profile appears centrally concentrated, with a gradual decrease in brightness moving outward from the core. The galaxy exhibits a generally elliptical shape, appearing more rounded than elongated. There is a subtle asymmetry in the outer regions of the galaxy, suggesting possible tidal interactions or recent minor disturbances. No distinct spiral arm structures or prominent dust lanes are discernible, but there is some evidence of clumpy regions in the central area. The object appears reddish in color. Overall, the morphology suggests a massive galaxy with a relatively low star formation rate. There may be subtle signs of past or ongoing mergers.
