The galaxy presents as a smooth, elongated structure with a high degree of central concentration. Its morphology appears to be that of an elliptical galaxy, lacking any apparent spiral arm features or significant dust lanes. The light distribution is fairly uniform, exhibiting a gradual decrease in intensity from the central core outwards. The core shows a yellowish hue, which may indicate an older stellar population dominated by red giant stars. No signs of active galactic nuclei activity are apparent in this image. Overall, the galaxy seems to be an evolved system with a smooth, regular profile, consistent with an elliptical classification.
