The galaxy presents as a largely spheroidal object. The light profile exhibits a centrally concentrated core with a diffuse, extended halo.  Color gradients are subtle, with the core appearing slightly more yellow/orange, suggesting an older stellar population.  The outer regions of the galaxy show hints of bluer tones, possibly indicative of more recent, though not particularly vigorous, star formation. No distinct spiral arm structures or dust lanes are discernible in the image.  The galaxy appears relatively undisturbed, showing no obvious signs of recent major mergers or tidal interactions. The overall morphology suggests an elliptical galaxy, although the slight bluing of the outer regions could indicate some ongoing, low-level star formation within a broader elliptical structure.
