The galaxy presents an overall elliptical morphology, appearing smooth with a centrally concentrated bulge. The core exhibits a yellowish-orange hue, suggesting an older stellar population and diminished ongoing star formation in the nuclear region. Fainter, bluish diffuse light extends outwards from the core, indicating the presence of a surrounding disk or halo component. There may be a faint disk present. The smooth appearance and color gradient suggest this is likely an early-type galaxy. There may be minor disturbances that could be indicative of a recent minor merger, but further investigation is required. 
