The galaxy exhibits a morphology that suggests a relatively smooth central component with notable disturbances. The primary body displays a roughly elliptical shape, with a brighter, more concentrated core. 

Extending from the main body is a faint, elongated tidal tail, suggestive of gravitational interaction with another galaxy. This tail appears diffuse and extends to a distance greater than the radius of the central body. There is an internal structure characterized by a central bulge. The galaxy’s color indices, revealed through the color gradients, may indicate varying stellar populations and dust content within the system.
