The galaxy appears to be a relatively compact object. The central region exhibits a smooth, bright profile, indicative of an elliptical or lenticular morphology. The light profile suggests a largely spheroidal component, with a high degree of radial symmetry. 

There is an irregular structure that is connected to the main body of the galaxy. This structure is more apparent away from the central body. This suggests the potential for an ongoing or recent merger event. There seems to be a tidal tail on the edge of the system.

Color variations are present within the galaxy. The central region appears more blue or white in color while the areas away from the center are more red. The color suggests varying stellar populations, with the bluer central regions indicating a potentially younger stellar population or ongoing star formation, while the redder regions potentially harbor older, redder stars.
