The galaxy appears as a somewhat elliptical, concentrated object. The central region exhibits a bright, yellowish-orange hue, suggesting a population of older stars. Extending outward from the core, a fainter, less defined halo is visible, exhibiting a bluer tint. The overall structure seems relatively smooth, lacking prominent spiral arms or strong dust lane features. There may be hints of slight disturbances in the outer halo, possibly indicative of minor gravitational interactions.
