The galaxy presents as a spiral type, characterized by a central bulge surrounded by a disk. The bulge appears moderately sized, exhibiting a yellowish hue indicative of an older stellar population. Spiral arms are discernible within the disk, although they are somewhat diffuse and not sharply defined. These arms display a bluer color, suggesting ongoing star formation regions within them. Faint indications of a bar-like structure seem to extend through the central region of the galaxy. The galaxy's overall structure appears relatively undisturbed, showing no obvious signs of a recent major merger event.
