The observed galaxy exhibits an elliptical morphology, appearing relatively smooth in texture. The concentration of light towards the center is high. The overall shape is approaching circular, without a significant disk structure that can be readily discerned, nor is there any evidence of spiral arms. The color profile of the galaxy is yellowish-orange, suggesting an older stellar population dominating its composition.

Based on the observations, there appears to be no significant signs of active galactic nuclei activity, nor is there evidence of ongoing star formation based on color. The galaxy does not exhibit any visual distortions indicative of recent or ongoing merger events. The overall appearance of the galaxy suggests a more evolved, quiescent system.
