The galaxy presents a largely smooth morphology, appearing generally elliptical in shape. Its core exhibits a concentrated luminosity, suggesting a high density of stars in the central region. The overall color profile indicates an aging stellar population, with a yellowish-red hue dominating the galaxy's light output. There is faint, diffuse light extending from the core with some very minor irregularities, which hints at possible disturbances or minor interactions. These disturbances appear as very faint, diffuse regions of somewhat different color. Overall, the galaxy appears to be a massive system, undergoing moderate star formation. The light output is consistent with an object at significant cosmological distance.
