The galaxy appears as a centrally concentrated object with a generally elliptical morphology. The light distribution suggests a relatively smooth profile. The color gradient is subtle, transitioning from a slightly redder core to bluer outer regions. There is a hint of disk-like structure, but this is not particularly prominent. Some minor disturbances or faint tidal features can be barely seen, suggesting potential past interactions. The absence of strong dust lanes further supports the relatively smooth nature of the galaxy. Star formation is likely present but at a modest rate given the lack of intense blue regions. Overall, the galaxy presents as a relatively evolved system.
