The galaxy presents as a concentrated elliptical form with a smooth luminosity profile. The core region exhibits a pronounced brightness, indicating a high stellar density and potential presence of a supermassive black hole actively accreting material. The isophotes appear elongated, suggesting a moderate degree of ellipticity rather than being perfectly spherical. The color is generally yellow and orange, which is indicative of a population of older, redder stars. There is no clear evidence of spiral arms, dust lanes, or significant ongoing star formation. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions in its recent past.
