The galaxy presents a largely smooth morphology, suggesting a dominant spheroidal component. It appears somewhat elliptical in shape, displaying a moderate degree of roundness, with subtle deviations from a perfect circular form. The galaxy exhibits a color gradient, appearing more yellow in the central region, potentially indicating an older stellar population and decreased star formation. There is little evidence of spiral arms or distinct disk features. No significant signs of tidal interactions, mergers, or major disturbances are readily apparent. The galaxy is relatively compact in size. Overall, the observed characteristics suggest a relatively evolved galaxy with a dominant bulge and a quiescent star formation rate.
