This galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing mostly round with only a slight elongation. The light profile indicates a bulge-dominated system, as the light intensity decreases gradually from the core. The central region has a yellow-orange hue, potentially indicating a population of older stars. A faint, greenish-blue halo surrounds the central bulge, suggesting the presence of some younger stars or ongoing star formation within a disk-like structure. There is no obvious evidence of spiral arms or strong tidal features suggesting a recent major merger event. The overall structure of this galaxy suggests it is a mature system, likely an early-type spiral or an elliptical galaxy.
