The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile is generally redder, indicating an older stellar population and reduced star formation activity. The galaxy exhibits a somewhat elongated shape, deviating slightly from perfect circularity. There are no discernible spiral arms or prominent dust lanes. The overall appearance suggests a galaxy that is nearing the end of its active star-forming phase, tending more toward a passive evolution. Evidence of minor tidal disturbance or interaction is possibly present, but it is difficult to determine conclusively due to the resolution of the image.
