This galaxy exhibits a prominent disk structure with a moderate-sized central bulge. Spiral arm features are discernible, though not sharply defined. There appears to be a bar-like structure present, although its strength is difficult to ascertain from this image alone. The galaxy does not present a clear edge-on profile. There is no evidence of ongoing major merging activity, although minor disturbances could potentially be present. The color profile suggests the presence of both older stellar populations in the bulge and relatively younger, bluer populations in the disk, particularly along the spiral arms.
