The galaxy presents a somewhat disturbed morphology, suggestive of an ongoing or recent interaction. The primary body of the galaxy appears roughly elliptical and its color is mostly yellow-orange. This implies an older stellar population and reduced star formation rate.

There is a secondary, smaller component which appears bluer in color than the main body, indicating the presence of younger, hotter stars. There is evidence of tidal features or distortions extending away from the main body, possibly indicating a merging event or gravitational disturbance. A significant fraction of smoothness suggests that it may become an elliptical galaxy upon fully merging with its companion. The galaxy has an estimated diameter of roughly 8.4 kpc, based on light distribution.
