This galaxy presents as a relatively face-on spiral, exhibiting a discernible but weakly defined disk structure. There is a subtle central bulge that appears smooth and brighter than the surrounding disk. The arms show signs of patchiness, with what could be regions of increased star formation activity. Overall, the galaxy has a somewhat hazy appearance, perhaps due to dust or a smooth stellar distribution within the disk. No obvious signs of a major merger event are apparent, although there may be some minor distortions within the disk's structure, suggesting possible interactions or past disturbances. The color profile indicates a mix of stellar populations, with a slightly bluer hue in the outer regions, indicative of younger, hotter stars.
