The galaxy presents as a somewhat smooth, centrally concentrated system. The light distribution appears relatively symmetrical and rounded, showing a lack of distinct spiral arms or a strong bar structure. There is a small degree of asymmetry in the overall shape. The galaxy exhibits a color gradient, with a slightly bluer periphery fading into a redder, more concentrated core. The core is the brightest portion of the galaxy. There is no strong evidence of ongoing major mergers or tidal disturbances in this image, although a possible minor disturbance or faint feature is suggested in the upper left portion of the galaxy's halo. Overall, it appears to be a relatively undisturbed system.
