The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated light profile. The core is characterized by a bright, yellowish-white hue, suggesting an older stellar population. Moving outwards from the center, the light gradually diminishes, with the outer regions displaying a more reddish tone. There's no clear evidence of spiral arms or significant dust lanes within the visible light. The overall shape appears roughly circular, with no obvious signs of major tidal disturbances or interactions with other galaxies. Minor asymmetric distribution in the luminosity appears, but does not seem to indicate an ongoing merger.
