The galaxy presents as an elongated, disk-like structure, oriented approximately vertically in the image. The central region exhibits a brighter, yellowish-white hue, suggesting a concentration of older stars. Fainter blue-ish regions extend outwards along the major axis, potentially indicating regions of ongoing star formation. There is some degree of visual asymmetry along the disk. Overall the galaxy appears relatively undisturbed, without obvious signs of major mergers or tidal interactions. The galaxy is not strongly resolved.
