The galaxy presents as a somewhat elongated structure with a concentrated central region exhibiting a smooth light distribution. The light distribution shows a color gradient with the center appearing to have a redder hue with a slight blue tinge overall. There is an indication of a possible tidal feature or minor disturbance present at the upper section of the galaxy, where the light appears fuzzier and extends further out, creating a slightly irregular halo effect. This region might be a sign of ongoing or past interaction with another galaxy. However, the overall morphology does not show the hallmarks of a major merger, rather hints at minor disturbances. The galaxy appears to be relatively compact in size, with a fairly symmetrical profile, besides the fuzziness at the top, suggesting an evolved system dominated by older stellar populations. There are not any defined spiral arms and the galaxy appears mostly smooth.
