The galaxy presents as a relatively smooth, centrally concentrated object. The core appears bright, with a yellowish-white hue, suggesting an older stellar population dominates the central regions. The outer regions of the galaxy exhibit a more diffuse, slightly bluer coloration, potentially indicating the presence of younger stars and ongoing star formation, although this is not strongly pronounced. There appears to be a slight asymmetry or faint extension to one side of the main body, hinting at possible tidal interactions or minor disturbances. The overall form suggests a late-type spiral galaxy or an elliptical galaxy with some ongoing star formation. There are no obvious spiral arm structures visible. The general morphology suggests the galaxy is in a relatively quiescent state, without a major ongoing merger event.
