The galaxy presents as a relatively small object with a disk-like morphology viewed at a high inclination, possibly nearing edge-on. Its overall structure is moderately elongated, with a clear central concentration that could indicate the presence of a bulge. The color profile exhibits gradients, suggestive of varying stellar populations. A blue tint is visible across much of the galactic disk, particularly around the edges, possibly indicating more recent star formation. There appear to be disturbances in the structure that are possibly signs of minor mergers.&#x20;
