This galaxy presents as an elliptical morphology, with a smooth, seemingly undisturbed structure. The galaxy exhibits a concentrated central bulge, characterized by a bright yellowish-orange hue, suggesting an older stellar population. The light intensity diminishes gradually from the core outwards, showing a smooth transition towards the galaxy's edges. There's a lack of defined spiral arms or dust lanes, further reinforcing the classification as an elliptical galaxy. The overall roundness of the galaxy indicates it is likely viewed close to face-on. Faint wisps of light extend beyond the core, potentially indicating a diffuse halo of stars. There appears to be no significant ongoing star formation.
