The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is generally round. There appears to be little to no evidence of spiral arm structure or a prominent disk component; any disk is likely viewed face-on. The galaxy exhibits a centrally bright core, surrounded by a more diffuse halo of light. Color gradients suggest a possible presence of older stellar populations. There are no immediately obvious signs of ongoing major mergers or significant tidal disturbances in its morphology. Evidence suggests its mass and size are typical. The galaxy appears to have a limited rate of star formation.
