The galaxy presents as a largely featureless, smooth elliptical galaxy, displaying a concentrated central bulge. The light profile appears to smoothly diminish from the core outwards. The galaxy exhibits a roughly circular shape, with a minor deviation towards a slightly elongated, or "in between", morphology. There is little evidence of spiral arms, bar structures, or dust lanes. The color gradient suggests a population of older stars, likely composed of primarily Population II stars, with reduced ongoing star formation. Faint tidal features are potentially present, indicating a possibility of a past minor interaction or merger event, however, no major disturbances can be seen.
