The galaxy presents as an elliptical or lenticular type, exhibiting a relatively smooth, concentrated structure. Its morphology is characterized by a prominent bulge, displaying a yellowish-white hue, indicative of an older stellar population. The outer regions of the galaxy show a gradual decrease in surface brightness, extending into a faint halo. There is a possible slight disk-like feature at the periphery. No distinct spiral arms or significant dust lanes are visible. The overall color suggests a lack of active star formation within the main body of the galaxy. The galaxy appears generally undisturbed with no signs of major mergers or tidal tails. There is a very slight asymmetry in the halo indicating a possible minor disturbance. The morphology is tending towards a spherical shape.
