The galaxy presents as a relatively smooth, centrally concentrated structure. The color profile indicates an older stellar population, particularly within the core region, which appears a yellow-red hue. There is a slight bluing of color away from the core, indicating younger stars. The galaxy demonstrates an elliptical morphology, deviating slightly from perfect circularity. No distinct spiral arm structures are visually apparent. There are hints of a faint disk present in the image, though it is largely obscured. There is no obvious sign of a major merger or strong tidal disturbances. It shows no bright star-forming regions are visible. Overall, this appears to be a relatively massive galaxy with a moderate rate of star formation.
