The galaxy appears as a centrally concentrated, elliptical-like structure. The light distribution is quite smooth, suggesting an older stellar population. There is a subtle color gradient visible, with the core appearing slightly more yellow/red than the outer regions, which could be due to variations in stellar populations or dust distribution. It exhibits a high degree of symmetry, indicating a relaxed morphology. There is no obvious evidence of spiral arms, disk features, or significant ongoing star formation activity. The general appearance of the galaxy is indicative of a relatively massive system that is not undergoing any major mergers or tidal interactions.
