The galaxy presents as a relatively compact object with a smooth, diffused light distribution. Its overall shape is approximately elliptical, tending towards circular, with no discernible spiral arm structures or a distinct central bulge. The light is centrally concentrated, decreasing gradually towards the edges. There are no obvious signs of a prominent disk component.

The galaxy exhibits a color gradient, appearing bluer in the central region and becoming slightly redder towards the outer regions, suggesting a potential variation in stellar populations. There are no clear signs of any ongoing major mergers or significant tidal disturbances, though subtle asymmetries or minor disturbances may be present within the light distribution. The galaxy does not display strong tidal tails or other signs of recent interactions.
