The galaxy presents a generally smooth morphology. The light distribution suggests an elliptical shape, though it is not perfectly round, appearing somewhat elongated along one axis. The core exhibits a brighter, more concentrated intensity. Surrounding the core, a fainter halo or extended envelope can be observed. The color profile indicates a population of older stars, with redder hues dominating the overall coloration. However, there appears to be a slight presence of blue light towards the central region, potentially indicative of a small amount of recent star formation or a different stellar population in that localized area. No distinct spiral arms or significant dust lanes are visible in this image, which further supports the classification of this galaxy as an elliptical type. There is no sign of ongoing mergers or major disturbances.
