The galaxy presents as a somewhat elongated, luminous structure. Its light profile appears relatively smooth, lacking any obvious spiral arm features or distinct dust lanes. The central region exhibits a brighter concentration of light, potentially indicating a prominent galactic bulge or active galactic nucleus. There is a suggestion of a disk-like morphology viewed at an inclined angle. The outer regions of the galaxy fade gradually, with no sharply defined edges. The color is predominantly blue-white, suggesting a population of relatively young, hot stars, although the lack of resolved stellar populations prevents a detailed analysis of its composition. Possible minor tidal disturbances are suggested by slight asymmetry in the outer halo.
