The galaxy presents a predominantly smooth morphology, indicative of an elliptical or lenticular type. Its light profile exhibits a centrally concentrated brightness, with a gradual decrease in intensity towards the outer regions. The galaxy core appears nearly spherical, with a slight elongation. 

The color of the central region tends toward a yellow-white hue, suggesting a population of older stars. Faint reddish regions, possibly regions of nebular emission, are present, one slightly brighter and more distinct than the others. No clear dust lanes or spiral arm structures are visible within the galaxy's body. There is no evidence of tidal tails or major morphological distortions, implying a relatively undisturbed evolutionary history.
