The galaxy presents a largely smooth morphology, appearing primarily as an elliptical or lenticular type. Its overall form is somewhat rounded but shows a slight elongation, verging away from a perfectly circular profile. There is no clear evidence of spiral arm structure or a prominent disk component. The galaxy exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions, but the edge is not well defined. Its color appears to be dominated by light at the redder end of the spectrum, suggestive of an older stellar population and relatively quiescent star formation. Faint signs of minor disturbances or interactions with other galaxies are observed.