The galaxy presents as an elliptical morphology, exhibiting a largely smooth light distribution without prominent spiral arm structures or a distinct galactic disk. Its color profile suggests a relatively older stellar population, with a yellowish-red hue indicative of evolved stars. The galaxy displays a moderate degree of central concentration, brightening towards the core. There is no obvious indication of ongoing major mergers or significant tidal disturbances. The overall shape tends towards a spheroidal form.
