The galaxy exhibits a largely elliptical morphology, with a relatively smooth, centrally concentrated light distribution. There is a subtle disk-like feature embedded within the larger elliptical structure, indicating potential spiral arm remnants or a flattened component. The galaxy's color profile suggests moderate star formation activity, with a slight blue tint to the central region. No distinct tidal tails or major morphological disturbances are immediately apparent. While a dominant, centralized bulge is prominent, the overall appearance points to a possible transition stage between a pure elliptical and a more structured spiral galaxy. The light is fairly uniform, however there are indications that there has been, or currently is, some interaction with another galaxy.
