The galaxy presents as a somewhat elliptical, smooth object with a concentrated central bulge. There is a subtle color gradient, transitioning from a more yellow-red hue in the core to a slightly bluer tint in the outer regions. No distinct spiral arms or other prominent features such as dust lanes are readily apparent. The overall morphology suggests a galaxy undergoing, or already having completed, a transition from a spiral to an elliptical form. The lack of significant morphological disturbances indicates relative quiescence, with no obvious signs of recent major mergers or strong tidal interactions. The estimated size indicates this is a substantial galaxy, and the colors suggest ongoing star formation. 
