The galaxy presents a predominantly smooth and rounded morphology. Its central region exhibits a concentration of light, suggesting a prominent galactic nucleus. A faint, diffuse halo surrounds the core, gradually fading into the background sky. There is some evidence of faint structures within the disk, possible spiral arms or tidal disturbances. The galaxy's color is generally yellowish, indicative of an older stellar population, but there are patches of bluer hues within the disk, suggesting more recent star formation activity. There is some indication of minor disturbance or interaction with a neighboring galaxy, but it doesn't appear to be a full-blown merger.
