The galaxy presents a relatively smooth, elliptical morphology. Its light is concentrated toward the center, displaying a bright, yellowish core which is consistent with an older stellar population. The outer regions exhibit a faint blue halo. There is little evidence of spiral arms or significant dust lanes, indicative of a system with a low rate of ongoing star formation. The overall structure appears undisturbed, showing no signs of major mergers or significant tidal interactions. The roundness indicates a morphology leaning towards E0-E3 on the Hubble sequence. Minor disturbances, such as the somewhat irregular outer structure, cannot be entirely ruled out. The galaxy seems to be in a relatively quiescent state.
