This galaxy exhibits a predominantly smooth morphology, with an apparent lack of distinct spiral arm structures or a prominent central bar. The overall shape approximates a rounded form, though subtle deviations from perfect circularity are present. There are hints of a disk-like component. The color profile suggests a moderate level of star formation activity within the galaxy, as indicated by a slightly bluer hue. Evidence of minor gravitational disturbances is observed, although major disruptions or ongoing mergers are not immediately apparent.