The galaxy presents a largely smooth and centralized morphology, suggesting an elliptical classification is appropriate. There appears to be a concentrated central bulge that exhibits a high degree of luminosity. There is a slight deviation from perfect circularity; the galaxy has a tendency toward a slightly elliptical shape. No significant signs of active galactic nuclei activity are immediately apparent in the visible spectrum. The galaxy does not exhibit any strong signs of spiral arm structures, major disturbances, or ongoing merger activity from the image. Given the color profile and shape, the galaxy likely has a relatively low ongoing star formation rate.
