The galaxy presents as a relatively smooth, elliptical-like structure with a slightly elongated morphology, exhibiting an intermediate roundness. The core region displays a yellowish hue, potentially indicating an older stellar population. A subtle gradient towards a greenish color can be observed in the outer regions, possibly indicating the presence of some younger stars or ongoing star formation, although this activity appears to be subdued. There is no evidence of strong tidal features or major disturbances, suggesting it is not currently undergoing a major merger event, although there may be signs of minor disturbances. The overall appearance is that of a relatively evolved galaxy with a significant fraction of its stellar population being old.
