The galaxy presents as an elongated, lenticular-like structure with a distinct central bulge. The disk component is observed edge-on, exhibiting a relatively smooth morphology, with an apparent lack of prominent spiral arms. The central bulge appears yellow-orange, suggesting an older stellar population dominating this region. The disk shows a color gradient, with a slight bluish tint towards the outer regions, potentially indicating younger, hotter stars and ongoing, though possibly subdued, star formation. No significant tidal features or signs of major mergers are discernible. The galaxy appears relatively isolated, with no immediately interacting companions visible in the immediate field of view.
