The galaxy presents as a somewhat diffuse, elliptical structure with a smooth luminosity profile, suggesting an older stellar population. It exhibits a slightly elongated shape, falling between a perfectly circular and cigar-like morphology. The galaxy's central region appears brighter and exhibits a yellowish hue, possibly indicating the presence of older, redder stars. Surrounding this core is a fainter, more diffuse halo with a hint of bluish coloration, suggesting the possibility of some ongoing, albeit limited, star formation. There appears to be no strong evidence of significant tidal disturbances or major mergers in this image, though minor interactions cannot be entirely ruled out based on the subtle irregularities in the outer halo. The overall appearance is consistent with a galaxy that is dominated by a spheroidal component, possibly an elliptical galaxy or a lenticular galaxy viewed close to face-on. The presence of the bluish halo warrants further investigation into its star formation rate.
