The galaxy presents as a roughly circular, centrally concentrated object. Its morphology is largely smooth, lacking significant disk features or spiral arm structures. The light profile indicates a dominant bulge component, appearing as a bright, yellowish core that gradually fades outwards. The lack of distinct features and the smooth light distribution suggests that the galaxy is relatively undisturbed, with no evidence of recent major mergers or significant tidal interactions. The galaxy exhibits a color gradient, transitioning from a more yellow hue in the central region to slightly redder tones in the outer parts. The moderate redshift and significant mass suggest that this is a mature galaxy with a relatively low rate of ongoing star formation.
