The galaxy presents a largely smooth and centrally concentrated morphology. The core region exhibits a bright, yellowish hue, indicative of an older stellar population. Moving outwards, the galaxy becomes more diffuse, with a subtle color gradient suggesting some ongoing, albeit low, star formation. There is a lack of distinct spiral arm structures or prominent dust lanes. Its overall shape is somewhat elongated, though not markedly so, suggesting it is somewhere in between a spherical and a highly flattened morphology. There are no clear signs of any major mergers or significant tidal disturbances. However, there appears to be a minor asymmetry, suggesting a potential past interaction or minor disturbance.
