The galaxy presents a somewhat amorphous morphology, with a luminous central region that appears relatively smooth. There is some indication of a disk structure, though it is not clearly defined. The shape of the galaxy appears somewhat in between round and elliptical, but more information would be needed to describe its exact morphology. 

There are hints of disturbances or interactions with other galaxies, which could indicate minor or major merging activities. These irregularities could be indicative of a non-equilibrium state.

The galaxy exhibits a distinct color gradient from its center towards its outer regions. The central region appears more yellow-orange, which could imply a higher concentration of older stellar populations or dust. The outer regions appear to possess more blue tones, which could be indicative of ongoing star formation or a younger stellar population. 

The apparent size of the galaxy is relatively small, indicating it's a distant object.
