The galaxy presents an elliptical morphology, exhibiting a smooth, symmetrical light distribution. The core region displays a concentrated luminosity, transitioning outwards to a less intense, diffuse halo. The observed color gradients suggest a variation in stellar populations, with the central bulge appearing redder, possibly indicating an older population of stars and a lower rate of ongoing star formation compared to the bluer, less concentrated outer regions. A slight disc may be visible in the outer regions with some star formation taking place. The galaxy does not display any signs of major disturbances or tidal features indicating any recent or ongoing major merging events.
