The galaxy presents as an elliptical structure, appearing largely smooth and spheroidal in shape with a high degree of roundness. The galaxy exhibits a prominent central bulge that gradually fades into a more diffuse halo, indicating a lack of significant dust lanes or spiral arm structures. The color gradient transitions from a yellowish-white core to a subtly redder outer region, potentially suggesting an older stellar population dominating the central regions. The apparent absence of blue colors indicates a low star formation rate. There is a nearby object that appears to be smaller and less dense than the primary galaxy. There are no signs of active galactic nuclei, such as prominent jets or outflows. The galaxy does not appear to be significantly disrupted or distorted, which would be an indication of a major merger event.
