The galaxy presents as a relatively smooth, elliptical-type object. It exhibits a concentrated central bulge, brightest in the visual spectrum, surrounded by a more diffuse halo. The color profile shifts from a yellow/white core, indicative of an older stellar population, to slightly bluer hues in the outer regions, which may suggest the presence of some younger stars or ongoing star formation. There is minimal evidence of spiral arms or significant dust lanes. The overall morphology suggests a relaxed system, likely devoid of any recent major merger events, though there may be slight disturbances visible.
