The galaxy appears to be relatively compact, exhibiting an overall elliptical morphology. The central region displays a concentrated luminosity, suggesting a prominent galactic nucleus. The light distribution indicates an intermediate axis ratio, with the galaxy appearing neither perfectly spherical nor highly elongated. There are some subtle features visible in the galaxy. The galaxy exhibits a relatively smooth appearance with little distinct spiral structure, with some disturbances in the outer regions. The lack of defined spiral arms and the overall smoothness suggest that the galaxy is probably a merging galaxy. A significant portion of the galaxy appears generally smooth and featureless, but there are some signs of more prominent star formation in its nucleus.
