The galaxy presents as a moderately bright, lenticular structure, exhibiting a centrally concentrated bulge that dominates its overall luminosity. The disk component is subtly apparent, with a flattened structure extending outwards from the central bulge. The galaxy appears relatively smooth in texture, lacking prominent spiral arms or significant dust lanes. Its color gradient suggests an older stellar population, with a yellowish hue dominating the central regions, indicative of evolved stars. No significant tidal features or signs of recent merger activity are discernible in this image, suggesting a quiescent state. The morphology suggests an intermediate stage between a spiral and elliptical galaxy. 
