The galaxy presents as a resolved object with an apparent elliptical morphology, though potentially with a disklike structure. There appears to be a central, bright nucleus, surrounded by a more diffuse halo of light. The color gradient suggests a slightly bluer central region transitioning to redder hues at the outskirts of the galaxy. There are hints of disturbed features within the galaxy's structure, possibly indicating a past interaction or minor merger event that may be influencing its overall morphology. The general smooth appearance suggests the presence of an older stellar population. There is low level star formation.
