The galaxy appears as a centrally concentrated, elliptical-like structure. Its core exhibits a strong reddish-orange hue, suggesting a relatively older stellar population and a scarcity of ongoing star formation in this region. Fainter, diffuse greenish light surrounds the core, extending outwards in an almost circular, smooth halo. This greenish outer region might indicate some residual, albeit low, levels of star formation, or potentially light from an active galactic nucleus. The overall structure lacks any distinct spiral arms or bar features. The object shows a high degree of central concentration, with light intensity diminishing gradually towards the outer edges. The galaxy does not appear to be undergoing any major merging activity or significant tidal disturbances.
