The galaxy presents as a spiral type, with a notable disk-like structure oriented close to face-on relative to our line of sight. Spiral arms are clearly visible, exhibiting a tightly wound morphology. A central bulge is apparent, though it appears relatively small compared to the overall disk size. The galaxy displays varying color intensities across its structure, with a brighter, yellower core region indicative of a high concentration of older stars. The spiral arms exhibit a bluer hue, suggesting ongoing star formation activity within the disk, albeit with what appears to be a low rate. The overall shape of the galaxy is elliptical, but flattened. There is no apparent bar structure. Evident is a small amount of asymmetry or minor disturbances. The galaxy's surface brightness profile appears smooth with no evidence of a significant merging event or other major interaction.
