The galaxy presents a generally smooth morphology, appearing largely elliptical in shape with a high degree of roundness. The central region exhibits a bright, concentrated core. The radial light profile appears relatively smooth, with the majority of the light concentrated in the center. There are some faint features, most likely tidal disturbances suggesting that the galaxy has recently experienced a merging event with another galaxy. This merger has likely fueled star formation in some regions of the galaxy. The colors are slightly redder in the core, indicating an older stellar population, whilst the fainter features that are less prominent are bluer, indicating the presence of younger, hotter stars in the outer areas.
