The galaxy presents as a predominantly smooth, elliptical structure with minimal discernible features. Its core exhibits a high degree of luminosity, transitioning to a more diffuse halo. There is a slight elongation to the morphology; it appears more oblate than spherical. The color profile indicates a generally older stellar population, with a greater concentration of redder wavelengths towards the center of the galaxy. There is limited evidence of spiral arms or active star formation regions within the visible spectrum. Small irregularities are visible, but their origin is ambiguous. These may be the result of past or ongoing minor merger events. Overall, the galaxy's appearance aligns with characteristics of a relatively evolved system.
