The galaxy exhibits a generally smooth morphology, with a slight elongation. Its color is predominantly yellowish-white, suggesting a population of older stars, although there are hints of bluer regions especially on the edges. The light distribution appears centrally concentrated. There are no prominent spiral arm structures or significant dust lanes readily apparent, indicating it is not a typical spiral galaxy. There is no clear evidence of tidal tails or other signs of recent major merger activity, though the slight asymmetry in shape might suggest a past interaction or minor disturbance.
