The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high degree of concentration with a yellowish-white hue, suggesting an older stellar population. There is a slight extension beyond this central region with a blueish tinge, though no distinct spiral arms or disk features are readily apparent. There appears to be no signs of a significant ongoing merger or major tidal disruption. Faint irregularities may suggest minor disturbances. The overall roundness implies a relatively low degree of flattening. Based on its color and form, this galaxy is likely a fairly massive system with modest levels of star formation.
