The galaxy presents a smooth, centrally concentrated morphology. Its overall shape appears largely elliptical, exhibiting a high degree of roundness. There is a distinct lack of prominent spiral arms or other complex features. The color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue in the central region. The outer regions of the galaxy display a slightly bluer tint, which could imply the presence of some younger stars, albeit in a relatively small fraction compared to the overall stellar population. No obvious signs of tidal disturbances or ongoing merger activity are detected from this view. The galaxy has an estimated median stellar mass between 10^10 and 10^11 solar masses, and a low star formation rate.
