The galaxy presents as a relatively smooth, elongated structure, exhibiting an elliptical morphology. It is characterized by a bright, concentrated central bulge that appears yellowish in color. Fainter, bluer extensions are observed emanating from the central region, suggesting the presence of a disk-like component. The disk structure exhibits a smoother texture, with hints of underlying substructure. Overall, the galaxy does not present with signs of major ongoing mergers or strong tidal disturbances, although there may be some subtle asymmetries in the disk indicative of minor gravitational interactions. The galaxy's color profile suggests a mature stellar population, but with potentially ongoing, low-level star formation in the bluer outer regions.
