The galaxy presents as a somewhat elliptical structure. The central region exhibits a high concentration of light, appearing nearly spherical and intensely bright, suggesting a significant population of older stars. Surrounding this core is a fainter, more diffuse halo that displays a subtle blue hue. The slight elongation implies it is an early-type spiral galaxy viewed at a small angle, a lenticular galaxy, or potentially an elliptical galaxy with some visible structure. There are very slight hints of a disk, indicating a possible transition between a spiral and elliptical morphology. The galaxy is relatively undisturbed, showing minimal signs of mergers or tidal interactions. The light distribution is relatively smooth, with no prominent star-forming regions discernible in this image.
