The galaxy presents an elliptical morphology, exhibiting a smooth light distribution that diminishes gradually from the central core outwards. The core shows a yellow/orange color, suggesting the presence of older stellar populations. A flattened disk-like structure is observed, oriented approximately horizontally in the image frame. The disk is a bluish color, which may suggest the presence of younger stars and ongoing star formation. The light distribution in the disk is not uniform, with some patchy areas along its edges, which is consistent with active regions of star formation. The overall shape appears to be significantly elongated, rather than circular. There is no clear evidence of spiral arms or other distinct morphological features beyond the central bulge and the flattened disk.
