The galaxy presents a generally smooth morphology, exhibiting a relatively uniform light distribution across its structure. It appears elliptical in shape, being more elongated than circular, with no discernible spiral arms or prominent disk features. The central region of the galaxy displays a higher concentration of light, suggesting a prominent galactic nucleus. There are hints of bluer regions mingled with the central yellow. The galaxy exhibits a red-shifted spectrum, indicating a considerable distance. Based on its smooth features, the galaxy appears to be a relatively mature system, possibly an elliptical galaxy with little ongoing star formation. There is minimal evidence of any major interactions or mergers affecting its current structure, though some minor disturbances cannot be ruled out.
