The galaxy appears to be an elliptical galaxy, exhibiting a largely spheroidal morphology. It presents a smooth, featureless appearance, with no discernible spiral arms or bar structures visible. The core is centrally concentrated and bright, suggesting a high density of stars and possibly an active galactic nucleus, although further spectral analysis would be required to confirm this. The galaxy exhibits a radial color gradient, transitioning from a yellowish-white hue in the core to a slightly redder tint in the outer regions. This color variation suggests an aging stellar population in the outer regions, indicating star formation occurred earlier in the galaxy's history. There is little evidence of ongoing star formation within the galaxy. The overall symmetry suggests that the galaxy is relatively undisturbed, with no major mergers or tidal interactions evident in this image, though a minor disturbance cannot be ruled out. The galaxy appears to be relatively massive and luminous, given its color and overall brightness.
