The galaxy presents a generally smooth and concentrated morphology, indicative of an elliptical galaxy. The central region exhibits a high degree of luminosity, appearing almost stellar-like, and transitions into a slightly fainter, diffuse halo. The overall shape is generally round with very faint wisps of a disk-like structure. There is no strong evidence of spiral arms or significant dust lanes. There appears to be only very minor disturbances to the structure, without strong signs of a major merger. Overall, the galaxy appears to be a relatively evolved system, consistent with a high mass and a moderate amount of star formation. The color profile suggests a redder population of stars, indicative of an older stellar population within the galaxy.
