The galaxy presents a largely smooth, elliptical morphology. The overall color profile is dominated by yellowish hues, suggesting a population of older stars. There is a slight elongation visible, although the galaxy is generally round in appearance. There is no apparent fine structure, such as spiral arms or dust lanes. A central bulge is clearly distinguishable, exhibiting a higher surface brightness compared to the outer regions of the galaxy. There's no visible evidence of ongoing major mergers or significant tidal disturbances affecting its shape. The galaxy's light is fairly concentrated, decreasing smoothly with radial distance from the central bulge.
