The galaxy presents a generally smooth and round morphology. A pronounced central bulge dominates the light profile, exhibiting a bright, yellowish-white hue. The outer regions of the galaxy gradually fade in intensity, displaying a slightly redder tint compared to the core, suggesting an older stellar population in these areas. There is a subtle hint of possible distortion or a minor disturbance in the overall symmetry, but nothing particularly notable, The galaxy appears to be relatively isolated, showing no immediately obvious signs of ongoing major interactions or mergers.
