The galaxy presents a generally smooth morphology, appearing elliptical in shape, with a high degree of roundness.  A slight elongation is noticeable, but the overall structure lacks distinct spiral arm features or a well-defined disk. Color gradients are subtle; the central region appears slightly brighter and more red, potentially indicating a higher concentration of older stellar populations.  The outer regions of the galaxy fade gradually into the background, suggesting a diffuse halo.  There is a strong likelihood the galaxy is currently undergoing, or has recently undergone, a merger event. There is no clear active galactic nucleus visible, and the relatively red color suggests a moderate to low star formation rate.  Based on its estimated size and luminosity, this galaxy is likely a massive system.
