The galaxy presents a generally smooth, elliptical morphology. It exhibits a high degree of central concentration, with the brightest region located at the core. This suggests an older stellar population dominates the central region. The galaxy appears slightly elongated. No distinct spiral arms or prominent dust lanes are visible. The overall color appears bluish-white, indicating a possible presence of younger stars, albeit not highly significant star formation activity. There is no clear evidence of recent or ongoing mergers or tidal interactions. The galaxy seems to be a relatively isolated system. The galaxy demonstrates a smooth gradient of light intensity decreasing outwards.
