The galaxy exhibits a disk-like morphology, with a notable tilt relative to the observer's line of sight. The overall structure is somewhat diffuse, with a central bulge region that appears brighter and more concentrated. Faint spiral arm features are visible, appearing somewhat flocculent and not sharply defined. The color profile indicates the presence of both younger, bluer stellar populations, particularly within the disk and arm regions, and older, redder populations, more concentrated toward the central bulge. There is a slight asymmetry or disturbance in the disk structure, potentially indicative of a past or ongoing minor merger event or internal dynamical processes.
