The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, transitioning to a reddish-orange tint in the slightly extended halo. There is no evident spiral structure or significant dust lane obscuration. Overall, the galaxy appears to be a relatively relaxed system, exhibiting little evidence of recent major mergers or significant tidal disturbances, though it may have some merging activity. The shape is mostly round. The galaxy appears to have a very low star formation rate.
