The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a bright, yellowish-white hue, indicating a likely concentration of older stellar populations. Moving outward from the core, the color transitions to a more diffuse, bluish-white, suggestive of a mix of stellar populations. There is a subtle disk-like morphology, with a relatively smooth texture. There is no clear evidence of significant spiral arm structures or active star-forming regions, although some patchiness is observed. No signs of major disturbances or merging activity are apparent, though a slight asymmetry cannot be ruled out. The overall appearance suggests a mature galaxy with a moderate stellar mass.
