The galaxy presents a relatively smooth and concentrated morphology. Its overall shape appears generally round. A distinct central bulge is visible, exhibiting a reddish hue, potentially indicating an older stellar population. The outer regions of the galaxy display a more greenish-yellow coloration, which could be indicative of ongoing, albeit subdued, star formation. There is no strong evidence of prominent spiral arms or bar structures, and the overall appearance suggests a relatively quiescent state. The galaxy does not show any obvious signs of major mergers or significant tidal disturbances.
