The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated, luminous core region that transitions gradually outward. The color profile suggests an older stellar population, indicated by the reddish-yellow hue concentrated at the center. There is evidence of a more diffuse, greenish halo surrounding the core which suggests there is likely some ongoing star formation, albeit at a lower rate. Overall, the galaxy appears as a fairly regular structure without significant signs of tidal disturbances or ongoing major mergers.
