The galaxy presents as a centrally concentrated, luminous object. Its overall morphology is smooth and elliptical, exhibiting a high degree of radial symmetry. The core region appears as a bright, unresolved nucleus, surrounded by a fainter, extended halo. There is a subtle color gradient visible, with the central bulge displaying a more yellow or gold hue, transitioning towards a slightly redder color in the outer regions of the halo. No distinct spiral arms, dust lanes, or significant morphological features are discernible, suggesting a lack of significant ongoing star formation within the disk and that it is composed of older stars. Overall, the galaxy exhibits a relatively undisturbed appearance, lacking any obvious signs of recent or ongoing mergers. The light distribution falls off gradually from the center, indicating a relatively smooth stellar density profile.
