The galaxy appears as a single, relatively smooth, and concentrated object. The color is predominantly a warm yellowish-orange. There is no strong evidence of spiral arms or a distinct disk-like structure. The object presents a slightly elliptical, though predominantly round, morphology. There are no prominent tidal tails or other signs of ongoing major mergers, although subtle disturbances cannot be ruled out. The galaxy exhibits a centrally concentrated light profile, diminishing in intensity towards the outer regions. The compact nature of the object is indicative of a significant, yet relatively quiescent, stellar population.
