The galaxy presents as a somewhat elliptical, disk-like structure with a moderate redshift. The color gradient indicates an older stellar population with a yellow-white core that fades into a redder periphery. There is a smooth distribution of light suggesting minimal dust lanes and a general lack of ongoing major star formation. The morphology appears relatively undisturbed, with no clear signs of recent major mergers, though there is potential evidence of minor disturbances in the outer regions. The overall shape leans toward being "in between" round and elongated.
