This galaxy presents as a predominantly smooth, centrally concentrated object. There is a distinct bulge component, exhibiting a yellowish-orange hue, that dominates the inner region. Extending outward from this central region is a fainter, more diffuse halo or envelope. The light distribution appears relatively uniform, lacking prominent spiral arms or dust lanes. There is a hint of a flattened disk structure. Overall, the galaxy's morphology suggests a relatively evolved system. There are no obvious signs of significant ongoing star formation or major disturbances. The galaxy appears relatively isolated, not showing clear signs of a major merger. Close inspection reveals a slight asymmetry or minor disturbances, which indicates some past interactions.