The galaxy presents as a moderately inclined spiral, exhibiting a central bulge that appears relatively smooth and concentrated. It demonstrates a disk component with hints of spiral arm structure, though the arms are not sharply defined, suggesting a flocculent morphology. The overall color index indicates a relatively evolved stellar population, with a discernible shift towards redder hues in the bulge and inner disk regions. There is evidence of ongoing, albeit modest, star formation, as indicated by the presence of some bluer regions in the outer disk. The galaxy appears to have experienced some level of past or ongoing gravitational interaction, as subtle distortions and tidal features are observed. The overall structure and color profile is consistent with a galaxy of intermediate mass and moderate star formation activity at a redshift of approximately 0.11.
