The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. Its overall shape is elliptical, tending towards a somewhat elongated form, but not significantly cigar-shaped. The light distribution suggests a dominant, relatively uniform stellar population across the galaxy. There's a suggestion of a slight colour gradient within the galaxy; the central region appears whiter, potentially indicating a population of older stars, with the outer regions trending towards a slightly bluer hue, implying the presence of some younger stars or ongoing, albeit low, levels of star formation. There are no readily apparent signs of spiral arms, bars, or significant dust lanes. There is no sign of strong tidal features or merger activity, instead, it exhibits a relatively undisturbed structure.
