The galaxy presents a largely smooth and rounded morphology. There is a concentration of light toward the central region, appearing as a bright, compact core. A surrounding, more diffuse halo extends outward from the core, diminishing in intensity with increasing radius.

There is some suggestion of a disklike component, though it is not very pronounced. We observe a moderate blue color, potentially indicative of ongoing star formation within the galaxy. There appear to be some minor disturbances in the outer regions, although a prominent merger is not present in the data. Overall, the galaxy appears to be in a relatively quiescent state.
