The galaxy appears to be an elliptical galaxy, characterized by a smooth, concentrated light distribution. The primary color is a yellow-red hue, suggesting an older stellar population with a lower rate of recent star formation. The galaxy has a relatively high degree of central concentration, with a clear, bright core. The galaxy exhibits a generally round morphology, lacking any prominent disk-like features or spiral arms. There are no obvious signs of ongoing mergers or major disturbances in its structure. Small disturbances may be present, but are difficult to interpret, given the resolution. The lack of blue color suggests a lower fraction of young, hot stars.
