The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a nearly circular morphology, with a notable absence of pronounced spiral arms or a distinct bar structure. The light profile appears to be dominated by a bulge-like component with a diffuse halo, indicating a considerable age and evolved stellar population. The color gradient appears to be minimal, transitioning from a yellow-orange center towards a slightly bluer outer region, indicative of a possible small level of ongoing star formation. There is no evidence of major mergers or significant tidal disturbances. The galaxy is a fairly massive galaxy, likely of an early type morphological classification, residing at a considerable cosmological distance and moderate redshift.
