The galaxy presents as a somewhat elliptical, likely disk galaxy with moderate redshift. It exhibits a bright, concentrated central bulge that appears yellowish, suggesting an older stellar population dominates this region. The disk component, while present, is less distinct and appears relatively smooth with subtle blue tints in the outer regions, which may indicate some ongoing, although comparatively low, levels of star formation. The overall morphology is dominated by a centrally concentrated light profile, and there is no visible evidence of strong tidal interactions or major mergers, although some minor disturbances cannot be ruled out based on the smoothness of the disk. The galaxy is moderately luminous, suggesting a substantial mass. The overall color indices point towards a more evolved system.
