The galaxy presents as a concentrated spheroid of light, indicating a dominant central bulge. The light distribution is relatively smooth, suggesting an elliptical or S0 classification. There is little evidence of spiral arms or significant dust lanes. Color gradients suggest a population of older stars, particularly in the galaxy's core. There appears to be some bluer light slightly offset from the center, possibly indicating some ongoing, low-level star formation. There are no apparent signs of major tidal disturbances or ongoing mergers in this image. The overall shape appears slightly elliptical, but close to round.
