The galaxy presents as a relatively smooth, centrally concentrated object with a slight ellipticity. The central region exhibits a bright, yellowish-white hue, suggesting a population of older stars. There is a subtle gradient in color and intensity as one moves outward from the center. The outer regions appear fainter and slightly redder, though there is a hint of bluer regions in the inner parts of the galaxy, possibly indicating some star formation. There is no clear spiral structure or prominent dust lanes visible. The overall morphology suggests an early-type galaxy, possibly an elliptical or lenticular galaxy, at a moderate redshift. The color profile implies an older stellar population dominating the galaxy's overall light output.
