The galaxy presents as a relatively small, elongated structure with a generally smooth appearance. There is a slight hint of a disk-like feature, though not clearly defined. The central region appears brighter and more concentrated compared to the outer edges, which gradually fade into the background. The galaxy's color suggests a mixture of stellar populations, with a possible dominance of older, redder stars. However, a faint hint of bluer light hints at some ongoing star formation. The galaxy does not display any major disturbances or signs of ongoing merging events, although minor irregularities in its shape cannot be ruled out. Overall, it seems to be an elliptical or lenticular galaxy that may be in the process of transitioning from a more active, star-forming state to a more quiescent one.
