This galaxy appears to be a relatively smooth, elliptical system, exhibiting a slightly elongated morphology. The central region displays a concentration of older stars, indicated by the reddish-yellow hue. Moving outwards from the core, a gradient towards green suggests the presence of a younger stellar population, likely from a lower level of star formation occurring within the galaxy. There are no obvious signs of spiral arms or a prominent disk structure. There are no signs of any major recent merger events or tidal disturbances of any kind. Overall, the galaxy presents an undisturbed appearance, indicative of a system evolving in relative isolation. 
