The galaxy presents a largely smooth, elliptical morphology with a centrally concentrated light profile. There is a subtle color gradient visible, with a slightly bluer hue towards the outer regions of the galaxy compared to the core, implying a potential difference in stellar populations. No distinct spiral arms or bar structures are discernible. There are subtle disturbances present implying a past minor merger. Its shape appears somewhere in between round and in between, with a slight preference to being in between. There is no major disturbance, and its features are mostly smooth. 
