The galaxy appears to be a relatively smooth, elongated object. It displays a moderate central bulge with a brighter, more concentrated core. The surrounding disk exhibits a slightly irregular shape. While a dominant spiral structure is not evident, there may be subtle signs of arms, or perhaps just a more diffuse, disturbed shape. The bluer regions are scattered in the galaxy, suggesting ongoing star formation. The overall color suggests that it is intermediate between a purely elliptical galaxy, where it is orange or red, and a blue spiral galaxy. There is no strong evidence of a major merger, but there is the possibility of a minor interaction. It exhibits moderate luminosity.
