This galaxy appears to be a relatively smooth, elliptical or lenticular type, exhibiting a centrally concentrated, bright bulge. The overall morphology suggests a spheroidal shape, with minimal discernible disk structure. The light distribution appears mostly uniform, lacking prominent spiral arms or distinct features typically associated with active star formation regions. The galaxy's color index, inferred from the red, green, and z-band data, suggests a population of older stars with little to no ongoing star formation. There may be some signs of tidal disturbances or a minor merger. Overall, the galaxy is characterized by a relatively smooth, early-type morphology with a dominant spheroidal component and a significant stellar mass.
