The galaxy presents as a somewhat smooth, centrally concentrated structure with a slight elongation. The central region exhibits a bright, compact core which gradually diffuses outwards. There's a subtle color gradient observed, with the core appearing slightly bluer compared to the outer regions which seem redder. Although largely smooth, there is some indication of subtle features in the outer disk, possibly suggestive of spiral arms or tidal disturbances. These features are not well-defined. Overall, the galaxy appears to be in a relatively quiescent state, with a moderate level of star formation. There is no evidence of major ongoing mergers, but some potential minor disturbances cannot be ruled out.
