The galaxy presents as a central, moderately bright concentration of light that appears relatively smooth in texture. Extending outward from this core are fainter, more diffuse regions of luminosity. The galaxy's shape is somewhat irregular, displaying a hint of a spiral structure, but with notable distortions and asymmetries. Some disruptions are visible in the galaxy's morphology, possibly due to tidal interactions with another galaxy. There may be an ongoing or recent merger event affecting the galaxy's overall form. Star formation appears to be low, given the absence of bright blue patches typically associated with young, hot stars, suggesting that it is either an elliptical galaxy, or a disk galaxy with little active star formation. 
