The galaxy presents a disk-like structure, viewed at a considerable angle. There is some evidence of possible distortion in its form. The central region appears bright and concentrated, suggestive of a prominent galactic nucleus. Proceeding outwards, the overall color profile indicates the presence of both younger, bluer stellar populations and older, redder populations. The disk shows mottled texture, potentially indicating regions of active star formation along its length, or dust lanes. The disk shows some features that could be evidence of tidal interaction or recent merger activity.
