The galaxy presents as an elliptical or lenticular structure, appearing largely smooth with a high degree of central concentration. The light distribution suggests an older stellar population, exhibiting a reddish-yellow hue. There is no readily apparent spiral arm structure or significant dust lane features. The galaxy displays a relatively uniform color gradient across its visible extent, with a slight increase in redder tones towards the core. The overall morphology suggests a galaxy that is well-evolved and quiescent, possibly experiencing a low rate of ongoing star formation. There are some minor color and luminosity fluctuations, but on the whole it appears to have a very smooth profile.
