This galaxy presents a generally smooth, elliptical morphology, displaying a centralized concentration of luminosity. The light distribution suggests a centrally dominant bulge component. The apparent roundness indicates a possible E0-E3 classification on the Hubble sequence, pending further kinematic analysis. Faint extensions are observed, possibly indicative of a weak disk component, but the lack of prominent spiral arms is consistent with the observed smooth classification. The galaxy appears to be fairly isolated with no clear major merger signatures, however some disturbance can not be ruled out. The color gradient from the center outwards shows the galaxy is redder in its core, and bluer in its edges. The lack of distinct features may also suggest the galaxy is in a quiescent state.
