The galaxy presents as a somewhat elliptical or lenticular morphology, appearing largely smooth and relatively featureless. The central bulge is prominent and displays a yellowish-white hue, suggesting an older stellar population with fewer young, massive stars. Moving outwards from the center, the disk or halo exhibits a gradual decrease in surface brightness. Faint blue tinges are present in the outer regions, possibly indicating some ongoing star formation, albeit at a low rate. There are no prominent spiral arms, bars, or obvious signs of a recent major merger event. Minor disturbances or faint tidal features may be present, but are not immediately apparent at this resolution. Overall, the galaxy appears to be a relatively evolved system with a moderate mass and a declining star formation rate.
