The galaxy presents a largely smooth morphology, appearing elliptical in shape, though not perfectly rounded, exhibiting a slight elongation. The central region displays a high surface brightness with a yellow-orange hue, indicative of an older stellar population. The outer regions fade gradually, showing a transition towards a bluer color, potentially signaling the presence of younger stars, or a lower concentration of dust. There is a hint of a possible minor disturbance on one side, suggested by a slight asymmetry or irregularity in the light distribution. The galaxy does not appear to be currently undergoing a major merger or exhibiting strong tidal features. Overall, the galaxy's structure suggests a relatively evolved system, possibly a transitioning stage between a disk-dominated and a spheroid-dominated morphology.
