The galaxy presents an elliptical morphology, with a bright, concentrated central bulge dominating the overall structure. The light distribution appears smooth, with no prominent spiral arms or distinct features visible within the galaxy's disk. There are two distinct areas of fainter, less concentrated light located to the side of the central bulge of the galaxy. The galaxy exhibits a color profile indicative of an older stellar population, appearing more yellow to red. The galaxy appears to be of significant mass, as evidenced by its luminosity and overall size. The rate of star formation is relatively low, which is also consistent with the galaxy's overall color and morphology. The galaxy appears isolated, showing no signs of major mergers or significant tidal disturbances. It exhibits a somewhat round shape.
