The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology. The central bulge is a prominent feature, displaying a concentrated luminosity. A faint disk component might be present, hinted at by a slight elongation and a subtle color variation across the galaxy's profile. The galaxy appears to be relatively isolated with no clear evidence of major mergers or significant tidal disturbances in the immediate vicinity, although a minor perturbation cannot be ruled out due to a slight lopsidedness. The color indices suggest the stellar population is moderately evolved, with a reduced rate of star formation within the galaxy's volume. The overall mass is estimated to be relatively high.
