The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an approximately circular morphology with no apparent spiral arm structures or distinct features indicative of a disk. There is a bright, yellowish core, likely indicating a high concentration of older stars within the galactic nucleus. The light gradually diffuses outward from the core, transitioning to a bluer hue in the outer regions. This color gradient suggests the presence of a younger stellar population in the galaxy's outer regions, possibly due to recent or ongoing star formation activity, although at a low rate. No signs of significant disturbances or ongoing mergers are apparent, and the galaxy appears relatively undisturbed. Based on its characteristics, this galaxy is likely to be an elliptical or lenticular galaxy at a moderate redshift.
