This galaxy presents as a somewhat elliptical, likely lenticular, structure. It exhibits a relatively smooth and centrally concentrated light distribution, suggestive of a dominant bulge component. There is little evidence of prominent spiral arms or significant dust lanes. The central region displays a yellowish hue, potentially indicative of an older stellar population. A subtle color gradient can be observed, transitioning from a slightly bluer color in the outer regions to a redder color towards the center. Based on the relatively high redshift, this is a galaxy a significant distance from us.
