The galaxy presents a largely smooth morphology, appearing elliptical in shape with a high degree of roundness. The central bulge is prominent, exhibiting a concentrated, bright yellowish-white hue. There's a subtle color gradient visible, transitioning to a bluer hue in the outer regions. The disk component, if present, is not clearly resolved in this image, which is consistent with the galaxy being of an early type. There are no obvious signs of major mergers or significant tidal disturbances in its structure. The lack of distinct spiral arms or prominent dust lanes further supports its classification as an early-type galaxy. The moderate redshift suggests that we are observing this object at a considerable cosmological distance. The overall light distribution is relatively even, with no significantly brighter or fainter spots except for the core, which could potentially indicate a more complex internal structure upon deeper inspection. The galaxy has a stellar mass in the range of 10^10 to 10^11 solar masses and the star formation rate is low.
