The galaxy presents as a face-on spiral with a moderately sized bulge. Spiral arms are clearly visible, exhibiting a three-arm morphology. The arms display a medium winding tightness. A bar-like structure appears present within the central region, with what seems to be a partial bar extending from the central bulge. No significant signs of tidal disturbances or ongoing major mergers are apparent in this image, however, there is a slight asymmetry, which may indicate a minor interaction. The spiral arms are well-defined and relatively smooth, with a noticeable color gradient shifting from bluer hues in the outer regions to a more yellow-red toward the central bulge. The central bulge appears luminous, with a concentrated light profile, indicating a significant stellar population.
