The galaxy exhibits a morphology suggesting an ongoing or recent interaction/merger event. The main body of the galaxy is relatively smooth and somewhat elliptical in shape, but it displays an irregularity in its structure. There is a secondary, smaller component that appears to be gravitationally bound to the primary galaxy. This smaller component is less defined and potentially tidally disrupted. The overall color suggests the presence of ionized gas, possibly indicating regions of active star formation. The shape is neither perfectly round nor elongated, placing it somewhere in between. There are also visible distortions suggesting tidal features resulting from the gravitational interaction.