The galaxy presents as a relatively smooth, centrally concentrated object with a faint but discernable disk. The overall color profile suggests a population of older stars, indicated by the dominant yellowish-orange hue in the central regions. There's a subtle hint of bluer regions within the disk, potentially indicating ongoing, but not necessarily vigorous, star formation. The galaxy's morphology appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. The galaxy appears slightly elliptical in shape, exhibiting a degree of rotational flattening. The outer regions fade gradually into the background sky, indicative of a diffuse halo surrounding the main body.
