The galaxy presents a largely amorphous morphology. It exhibits a smooth profile, with the light concentration appearing relatively centralized. There is a slight elongation, but the overall form is mostly circular. There is no clear spiral structure visible. Subtle variations in luminosity are present, but no dominant features, such as tidal tails or distinct nuclei, are observed. The faintness of the outer regions suggests a gradual decline in stellar density with increasing radial distance from the center. No features are suggestive of a major or minor merger event, though some minor disturbance cannot be completely ruled out. The light emitted is fairly uniform, with some slight differences in the green-red wavelengths.
