The galaxy presents as a single, somewhat amorphous object. There appears to be evidence of two distinct central concentrations of light, suggesting the possibility of a recent or ongoing merger. The overall shape is fairly round, although some distortion is apparent, possibly related to tidal interactions.

The light distribution is relatively smooth, with a gradual decrease in intensity from the core outward. This suggests that the galaxy may be an elliptical or lenticular type galaxy. There are no prominent spiral arm structures visible. The color appears yellowish-white in this image. There might be some minor irregularities in the outer regions, hinting at potential tidal debris or faint stellar streams associated with past interactions.
