The galaxy presents a distinct spiral morphology, with a discernible disk structure. Spiral arms are clearly visible, exhibiting a somewhat patchy distribution of light, suggestive of ongoing star formation regions within the arms. The galaxy displays a notable central bulge, appearing relatively prominent and possessing a smooth, concentrated light profile. The overall color gradient suggests a population of older stars concentrated in the bulge, with bluer hues apparent in the disk, consistent with younger stellar populations. No significant tidal features or signs of recent major merger events are immediately apparent, although some minor disturbances or asymmetries within the disk cannot be ruled out based on this image alone. The disk is oriented at a shallow inclination relative to our line of sight.
