The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge which dominates the overall structure. The light profile decreases radially from the center, exhibiting a gradual fade towards the edges. There is little evidence of prominent spiral arms or a distinct disk-like structure. The overall shape is slightly elongated, deviating marginally from perfect circularity. No significant dust lanes or star-forming regions are apparent. The overall color suggests an older stellar population, with a predominantly yellow hue. The galaxy seems to be fairly isolated, with no signs of ongoing major mergers or tidal disturbances.
