The galaxy presents a generally smooth, elliptical morphology. There is an absence of prominent spiral arm structures or a well-defined disk. The light is concentrated towards the center, suggesting the presence of a significant bulge component. The overall color is redder, with the core appearing more yellow, indicating an older stellar population and relatively low levels of ongoing star formation. There is evidence of a possible interaction or merger event, exhibiting a disturbed morphology or tidal features. There is some distortion of the light in the galaxy, suggesting it is being influenced by something else nearby, like a merging galaxy.
