The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is approximately elliptical, with a slight elongation suggesting a transition between elliptical and lenticular morphology. The color profile appears predominantly red, indicating an older stellar population with reduced ongoing star formation. There may be some slight irregularities in the overall light distribution, suggesting possible past interactions or minor disturbances, though there is no clear evidence of a major merger. The overall appearance is consistent with a massive galaxy with suppressed star formation.
