The galaxy presents as a somewhat smooth, centrally concentrated object with a slight elongation. It appears relatively featureless, lacking prominent spiral arms or a distinct bar structure. The color distribution suggests a dominant population of older stars, indicated by the redder hue, although there are some hints of bluer regions that could indicate ongoing star formation. There is a hint of disturbance with possible merging in the form of some irregular features. The overall morphology indicates a galaxy that may be transitioning toward an elliptical shape, possibly following a merger event.
