The galaxy presents as a roughly elliptical or lenticular structure, exhibiting a central, bright bulge that appears yellowish, indicative of an older stellar population. The outer regions of the galaxy display a bluer hue, suggesting the presence of younger stars and possible ongoing star formation. There is a hint of faint, diffuse spiral arm structure in the outer disk, although it is not sharply defined. The morphology suggests a galaxy somewhere between a pure elliptical and a more developed spiral, perhaps an Sa or Sb type. The relative smoothness of the galaxy indicates it is not undergoing a major merger event, although there might be some minor tidal interactions that have resulted in some asymmetry of the outer disk. The overall color profile suggests a galaxy that is transitioning from an active star-forming phase to a more quiescent state.
