The galaxy presents as a relatively compact object with a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. There is a concentration of light toward the center. The color distribution suggests a potential for older stellar populations, with a subtle reddening toward the central region. A very subtle disk structure may be present. There appears to be little to no ongoing major star formation present, though there may be low levels of star forming activity. There is no obvious sign of interactions with nearby galaxies or significant tidal disturbances. Overall, this is likely a galaxy that has undergone the bulk of its merging activity.
