The galaxy presents as an elongated, lenticular-like structure. The central bulge is prominent, exhibiting a concentrated luminosity with a yellowish hue, suggesting a population of older stars. There is a smooth transition from the bulge outward, with a gradual decrease in brightness toward the edges of the galaxy. The disk appears relatively featureless, lacking any distinct spiral arm structures. The overall color gradient indicates a potential decline in star formation activity from the center outwards. The galaxy appears to be generally isolated with no signs of tidal disturbances or nearby companion galaxies. The morphology suggests a transition type between a spiral and elliptical galaxy, potentially nearing the end of its star formation phase.
