The galaxy appears to be a merging system, consisting of at least two distinct components. The primary component is a relatively smooth, spheroidal object, with a concentrated core emitting strongly in the blue wavelengths. This suggests a high concentration of hot, young stars or a possible active galactic nucleus.  A secondary component is present, showing a more diffuse and elongated morphology and emits strongly in redder wavelengths. This suggests a greater presence of older stars or dust. There appears to be some distortion or tidal features around the redder object, indicating a potential interaction between the two systems. The overall shape of the galaxy system appears roughly circular, although this may be influenced by the ongoing merger process.
