The galaxy presents a flattened, elongated morphology, suggesting it may be classified as a spiral galaxy viewed edge-on or possibly an elliptical galaxy with a prolate shape. There is a distinct central bulge that appears yellowish-white in color, potentially indicating an older stellar population or a significant amount of dust obscuring bluer light. The outer regions of the galaxy show a fainter, bluer hue, suggesting younger stars and ongoing star formation within a disk-like structure. The system does not show any strong signs of tidal interactions or major disturbances, although there is a slight asymmetry in the distribution of the light in the outer regions which could suggest a previous minor interaction or accretion event. Overall, the galaxy appears relatively smooth, with a dominant spheroidal component and a fainter disk.
