The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. It exhibits a generally round morphology, with minimal discernible features such as spiral arms or a pronounced disk structure. The light distribution is dominated by a bright, central bulge, indicating an older stellar population and a lack of significant recent star formation. The galaxy appears to be relatively isolated, without any obvious signs of ongoing or recent mergers with other galaxies. The overall color is somewhat redder, suggesting a population dominated by older, redder stars with lower levels of current star formation. A slight asymmetry is present in the outer regions, but this is not enough to indicate a significant interaction or disturbance.
