The galaxy presents as a relatively smooth, elongated structure. The light distribution appears concentrated towards the center, suggesting a prominent bulge. The overall color gradient shifts from a slightly bluer hue in the outer regions to a more reddish-yellow tone toward the central bulge. This color variation could indicate differing stellar populations, with potentially younger, hotter stars in the periphery and older, cooler stars dominating the central region. There is no apparent spiral structure or distinct dust lanes visible within this image. The galaxy appears relatively isolated, without obvious signs of tidal disturbances or ongoing mergers with other galaxies.
