The galaxy presents as a moderately luminous, well-defined elliptical structure. Its morphology appears largely smooth, with a high degree of central concentration. Color gradients are subtle, suggestive of an older stellar population. The ellipticity is not extreme, displaying a generally rounded form. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity, though a fraction of features point to minor disturbances. Overall, it appears to be a relatively undisturbed system.
