The galaxy presents a primarily smooth, elliptical morphology, with an overall color gradient from a central bluish-white region to a more yellowish-red periphery. The central region is brighter and denser, suggesting a concentration of older stars. The overall shape appears to be moderately elongated, approaching a cigar-like morphology. There is a subtle suggestion of minor disturbance or tidal features, indicating a possible past interaction or minor merger. The presence of the redder component on the edge suggests a potential site of more intense star formation or the influence of dust obscuration.
