The galaxy presents as a relatively smooth, elliptical morphology. The light profile suggests a concentrated central bulge, surrounded by a more diffuse halo. There is little evidence of distinct spiral arm structure or significant dust lanes. The galaxy appears somewhat rounded in shape, deviating slightly from a perfect circle. There is no obvious signature of major ongoing mergers, though a very slight disturbance is possible in the surrounding halo. Color gradients suggest that the central region is dominated by older stellar populations exhibiting yellow and redder hues. The outer regions show fainter bluer colors, suggestive of more recent, less prominent star formation activity. The object is relatively compact, occupying a small angular size in the frame. 
