The galaxy presents as a centrally concentrated object with a generally smooth appearance, displaying a slight elongation. The color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue concentrated within the galaxy's core. There's a subtle transition toward bluer colors in the outer regions, potentially indicating more recent star formation activity, albeit at a lower rate. The overall structure hints at a relatively evolved system, showing only minor indications of disturbances or interactions.
