The galaxy presents as a single, relatively smooth object with a concentrated central region. The morphology is primarily elliptical or spheroidal, displaying a high degree of circularity. There's no significant evidence of spiral arms or a prominent disk structure. The galaxy core exhibits a noticeable brightness, indicating a potentially dense stellar population in the nuclear region. Based on its overall appearance, star formation is likely suppressed. No signs of major mergers or tidal disturbances are evident.
