The galaxy exhibits a pronounced disk-like structure, presented at a moderate inclination. The central bulge appears prominent, contributing significantly to the overall luminosity. Faint spiral arm structures are suspected, though not distinctly resolved in this image. The disk appears moderately smooth in texture, indicating a possible mix of older stellar populations throughout its structure. A bar structure appears to exist along the center. No significant tidal features or distortions are apparent, suggesting the absence of any recent major merger events. The galaxy's overall color suggests it is a relatively mature system with a moderate amount of on-going star formation.
