The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, bright central bulge, which dominates the galaxy's luminosity. The outer regions appear more diffuse with a slight elongation in its overall shape. Faint blueish hues are subtly visible in the outer regions, suggesting the presence of some star formation, but the galaxy as a whole appears to be composed primarily of older stellar populations. There's no strong evidence of spiral arm structure, or any significant merger activity or tidal disturbances in the immediate vicinity, although there are some subtle irregularities. The color distribution is fairly uniform across the galaxy, with the central bulge slightly redder than the outer regions. The galaxy appears relatively isolated, with no other obvious galaxies nearby that are currently interacting with it.
