The galaxy presents as a somewhat irregular or disturbed system, exhibiting a non-uniform distribution of light. It has a dominant central bulge and appears mostly smooth. Hints of a possible disrupted disk are visible, with some asymmetric extensions of the galaxy. The galaxy's light profile suggests that it is somewhere in between round and elliptical. The bluer color and irregular morphology suggest a population of young, hot stars and ongoing star formation, as well as a potential history of interactions or a recent minor merger event. The central region is relatively concentrated in brightness, which is typical of galaxies with smooth central structures. The overall appearance and disturbance of the galaxy suggests the possibility of internal processes and external interactions.
