The galaxy presents as a spiral type, viewed at a slight angle that is not quite face-on.  Spiral arms are visible, though not sharply defined, extending from a central bulge. The arms appear somewhat flocculent, exhibiting a patchy distribution of stellar populations. A central bulge dominates the galaxy's luminosity. The disk is relatively extended, showcasing a smooth distribution of light, but there are no obvious disturbances or indications of interactions with neighboring galaxies, but minor disturbances cannot be ruled out. The galaxy exhibits a color gradient, with the central bulge appearing yellower and the spiral arms exhibiting a bluer hue, suggesting ongoing star formation within the disk. A bar is possibly present within the central region, though it is not strong. 
