The galaxy presents as a single, relatively smooth object with a concentrated central region. The overall color appears to be yellowish-orange, indicating a population of older stars. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy appears approximately round in shape, showing a high degree of central concentration, and a slight elongation is possible. There appears to be little evidence of any major tidal disturbances or ongoing mergers. There is perhaps a slight asymmetry to the overall structure, suggesting a possible past interaction, but the galaxy presents a fairly relaxed morphology.
