The galaxy presents as a slightly elongated, disk-like structure, viewed at an oblique angle. Its central region appears significantly brighter and more concentrated, suggesting a prominent galactic bulge. The bulge exhibits a smooth, even texture with a slightly yellowish tinge. Emanating from the core are fainter, bluish, diffuse arms that extend outwards, but these lack the distinct spiral arm structure of a typical spiral galaxy. There is a subtle hint of asymmetry in the outer regions of the disk. The galaxy appears relatively undisturbed with no large tidal tails or obvious signs of an ongoing major merger event. The smooth, homogenous appearance suggests a relatively old stellar population dominating the light output, especially within the central bulge. Some bluer tones are visible, indicating regions of ongoing star formation, but these are not particularly prominent. Overall, the galaxy appears to be a transitioning system, potentially evolving from a spiral towards a more lenticular or elliptical form.
