The galaxy presents a centrally concentrated morphology, exhibiting a relatively smooth and somewhat rounded appearance. There is a notable absence of well-defined spiral arm structures or a prominent disk. The light profile suggests a spheroid-dominated system, with a gradual decline in brightness from the core outwards.

Color gradients are observed within the galaxy. The central region displays a yellowish hue, likely indicative of an older stellar population and/or the presence of dust. Fainter reddish patches appear slightly offset from the core, potentially indicating pockets of on-going or recent star formation. The overall color suggests the galaxy is at a significant redshift.

There appear to be some minor morphological disturbances or irregularities in the galaxy's overall shape, suggesting it may be undergoing some form of interaction or merging event. However, these disturbances are not severe, and the overall structure remains relatively coherent.
