The galaxy presents an overall smooth morphology, with a slight elongation. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is a hint of a disk-like structure, though it is not prominent. The color appears to be a relatively uniform, slightly bluer hue, suggesting ongoing star formation. There may be some minor disturbances in the galaxy's structure. The galaxy does not appear to be undergoing a major merger.
