The galaxy presents as a largely smooth, centrally concentrated object. The core region exhibits a yellowish-white hue, suggesting an older stellar population is dominant. Moving outward from the center, a subtle bluish-green halo extends around the core. This may indicate the presence of a younger stellar population and/or ongoing, low-level star formation within this region. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The light distribution is roughly circular, with only slight deviations from perfect symmetry. It is moderately luminous, but not exceptionally bright.
