The galaxy presents as an elliptical or lenticular type. It has a smooth, centrally concentrated light distribution, with a bright, relatively large bulge dominating the structure. There is little evidence of spiral arms or significant dust lanes. The galaxy appears to be generally round in shape, exhibiting a slight elongation. The color profile suggests the presence of an older stellar population within the bulge, indicated by the yellow and reddish hues. There may be evidence of minor tidal disturbances or interactions. The overall morphology indicates a galaxy that has undergone significant evolution.
