The galaxy presents a predominantly smooth, elliptical morphology. The light distribution is centrally concentrated, with a gradual decrease in surface brightness moving outwards from the core. The galaxy displays a color gradient, transitioning from a yellowish-white core to reddish hues in the outer regions. This suggests a potential decline in younger stellar populations and/or increasing dust content towards the periphery. There appears to be a very minor asymmetrical feature or tidal disturbance present on one side of the galaxy, which could potentially be the result of an interaction with another galaxy or a minor merger event. The overall shape appears generally rounded, with no clear spiral arm structures visible.
