The galaxy appears as a centrally concentrated, smooth object. Its morphology is broadly elliptical, showing a nearly circular isophotal shape. There is a slight elongation, but no obvious disc structure. The galaxy exhibits a dominant yellow-orange color gradient, suggesting a relatively old stellar population, likely dominated by evolved stars. There are no visible signs of active star formation regions, such as blue knots or HII regions. No strong dust lanes or tidal features are observed, which could indicate a past or ongoing merger event, however, there may be a small disturbance. The light distribution appears relatively symmetric and undisturbed, indicative of a stable and relaxed system.
