The galaxy presents as a largely featureless elliptical or lenticular type. It exhibits a smooth, concentrated light profile, with a centrally dominant bulge. There is no clear evidence of spiral arms, dust lanes, or prominent star-forming regions. The color is relatively uniform, with a yellow-red hue indicative of an older stellar population. There is a slight elongation in shape, but the galaxy appears mostly spheroidal. The overall impression is of a mature system that is not undergoing significant current star formation. There is no indication of recent merging activity, nor are there signs of tidal tails or other disturbances in the immediate vicinity. The light is somewhat dim, which could be due to distance.
