The galaxy presents an overall smooth morphology, appearing elliptical in shape. It exhibits a concentrated central bulge which graduates outward into a less dense halo. The color profile shifts from a yellow/golden hue at the core towards a bluer periphery, possibly indicating a difference in stellar populations. No distinct spiral arms or dust lanes are readily apparent, and the galaxy seems to be relatively undisturbed, with no major signs of ongoing mergers or significant tidal interactions. There may be subtle indications of minor structural disturbances, potentially signifying past interactions, but these are not prominently displayed.
