The galaxy appears to be a relatively smooth elliptical type, displaying a concentrated central bulge that gradually fades into a diffuse halo. The core exhibits a slightly reddish hue, which suggests an older stellar population dominating the region. Moving outward from the core, the galaxy transitions to a faint greenish color, indicating the presence of some younger, hotter stars, although they appear to be a small fraction of the galaxy's total population. The galaxy exhibits a high degree of radial symmetry, with only minor deviations from a perfectly elliptical shape. There is no obvious evidence of spiral arms or a prominent disk. The galaxy does not appear to be undergoing any major mergers or significant disturbances.
