This galaxy exhibits a clear disk structure, viewed at a significant inclination relative to our line of sight. The presence of spiral arms is evident, though somewhat ill-defined; they appear flocculent, lacking grand design characteristics. The color profile suggests ongoing star formation, with bluer regions concentrated within the spiral arms. A central bulge component is discernible but appears relatively small compared to the overall disk size. There is visual evidence for a bar-like structure extending through the central region.  The galaxy appears to be undergoing some form of interaction or disturbance, potentially a minor merger, as indicated by an asymmetry in the disk and/or tidal features. Overall, it presents as a late-type spiral galaxy with moderate star formation activity and subtle indications of tidal interaction.
