The galaxy appears as a single, relatively smooth object. The light profile suggests it has a centrally concentrated bulge, with light gradually decreasing toward the outer edges. The galaxy is roughly elliptical, tending towards an intermediate level of roundness. The overall structure indicates that the galaxy is not experiencing major ongoing merger activity. However, there are some minor potential disturbances that could be subtle signs of an interaction, possibly in the form of tidal features around the galaxy. The color gradients across the galaxy are not prominent, suggesting a relatively uniform stellar population. There may be some evidence of a feature or disk that is embedded, but the morphology is still dominated by a smooth component.
