The galaxy presents as an elliptical or possibly a lenticular galaxy, exhibiting a generally smooth morphology with little evidence of distinct spiral arms or significant dust lanes. The light distribution is centrally concentrated, indicating a relatively old stellar population, with a yellowish-orange hue predominating in the core region. The outer regions of the galaxy appear fainter and bluer, suggesting the presence of some younger stars or a small amount of ongoing star formation, although the overall rate appears to be low. The galaxy exhibits a slight elongation, deviating somewhat from a perfectly circular shape. No signs of major mergers or significant tidal disturbances are apparent; however, there may be a minor asymmetry to the overall structure suggesting a past interaction or minor disturbance.
