The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth, centrally concentrated morphology. The central bulge is prominent and appears yellowish-white in color, indicating an older stellar population. There is a faint disk-like structure surrounding the bulge, though details are difficult to discern, possibly due to distance. No distinct spiral arms or strong star-forming regions are visible. The galaxy appears relatively undisturbed, with no clear signs of recent major mergers or tidal interactions. There is a slight asymmetry in the outer regions of the galaxy. Overall, the galaxy appears to be a mature system with a relatively low rate of ongoing star formation.
