The galaxy presents a generally smooth morphology, suggestive of a relatively evolved system. It exhibits a flattened, elliptical shape, leaning towards a more elongated profile rather than perfectly circular. The central region displays a bright, concentrated bulge, indicating a high density of stars likely composed of an older stellar population. The color of the bulge appears yellowish-orange, consistent with older, cooler stars dominating its light emission. The outer regions of the galaxy display a faint, hazy disk. There is evidence of subtle internal structure, perhaps suggestive of faint spiral arms or dust lanes, however these features are not sharply defined. The overall color gradient transitions from the warmer central bulge to cooler, bluer tones in the outer disk, which implies the potential presence of younger, hotter stars and ongoing star formation. No significant signs of tidal disturbances, major mergers, or strong interactions with other galaxies are apparent in the image.
