The galaxy exhibits an elliptical morphology, appearing relatively smooth with no discernible spiral arms or bar structure. It presents a concentrated central bulge, characterized by a bright, yellowish-white hue, suggesting a population of older stars. The galaxy's overall shape is slightly elongated, indicating a non-circular structure with an axial ratio close to 0.9. The outer regions of the galaxy fade gradually into the background, forming a faint halo. The galaxy's colors become redder at greater radii, hinting at radial population gradients within. The galaxy is estimated to be more than 15 billion solar masses. The colors observed suggest star formation is fairly low, but may be observed in the center.
