The galaxy presents a generally smooth and elliptical morphology. Its light profile appears centrally concentrated, displaying a bright core that gradually fades towards the outer regions. The observed color is predominantly yellow-red, suggesting a stellar population dominated by older, evolved stars with relatively low ongoing star formation. There is a subtle, though present, hint of a disk shape in the galaxy, though this is not very prominent. No spiral arm structure or significant dust lanes are readily apparent. There are no visible signs of any major ongoing merger or significant tidal disturbance. Overall, the galaxy seems to be a relatively undisturbed system, with little to no recent star formation or interactions.
