The galaxy appears to be undergoing a merger, characterized by two distinct, luminous components with a moderate amount of tidal disturbance. The overall structure presents as irregular with a generally elongated shape. The components exhibit an orange-red hue, suggesting an older stellar population and lower star formation rate. No spiral arm structure is readily apparent. The central region of the galaxy is difficult to assess due to the ongoing merger, however, distinct centers of light are visible. The outer regions display faint extensions, indicative of tidal tails or debris resulting from the gravitational interaction. The galaxy's estimated size is about 4 Kpc, which is relatively small.
