The galaxy appears as a relatively compact system with a somewhat smooth morphology. It exhibits a generally elliptical shape, showing a slight elongation. There may be some faint disk features. The galaxy's light profile seems centrally concentrated, with a gradual decrease in intensity towards the outer regions. Color gradients across the galaxy suggest variations in stellar populations. The central region appears more yellowish and red, potentially indicative of older stars, while the outer edges may have bluer hues, suggesting the presence of younger stars. The galaxy does not show strong signs of ongoing major mergers, although subtle disturbances or minor tidal features may be present.
