The galaxy presents as an elliptical or lenticular type, with a smooth, concentrated light profile. The central bulge exhibits a yellowish hue, indicative of an older stellar population. There is a noticeable decrease in luminosity towards the outer regions of the galaxy, with the color gradually shifting towards a redder, less intense shade. No distinct spiral arms or prominent dust lanes are apparent within the galaxy's structure. There is some subtle evidence of minor disturbance. The overall morphology suggests a system with relatively low ongoing star formation.
