The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge exhibiting a yellow-white hue, suggesting an older stellar population. The surrounding halo appears fainter and more diffuse, transitioning gradually into the background. There is minimal visible structure, such as spiral arms or dust lanes, indicative of a lack of significant ongoing star formation. The overall shape appears nearly circular, with no obvious signs of tidal disturbances or ongoing mergers, though subtle asymmetry cannot be entirely ruled out at this resolution. The color gradient suggests a redder outer halo compared to the central region, potentially indicating a radial age or metallicity gradient within the stellar population.
