The galaxy presents a primarily smooth morphology, with no strong evidence of spiral arms or prominent dust lanes visible at this resolution. Its overall shape appears somewhat elliptical but tending towards a more intermediate disk-like structure, appearing neither perfectly spherical nor highly elongated. The central region exhibits a brighter, more concentrated luminosity, suggestive of a galactic bulge. There is a subtle color gradient across the galaxy, with the central bulge tending towards yellower hues, potentially indicating an older stellar population. The outer regions display a slightly bluer tinge, hinting at the presence of younger, hotter stars, albeit with less star formation observed currently. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions.
