The galaxy presents a primarily smooth morphology, appearing largely spheroidal in shape with a high degree of roundness. There is evidence of a central bulge with a higher concentration of luminosity, gradually decreasing outward. The overall color of the galaxy is consistent with an older stellar population, exhibiting a yellowish-red hue in the central region. Subtle indications of minor disturbances exist within the galactic structure, although no major mergers or violent interactions are immediately apparent. Faint outer regions indicate a larger radius of influence, but these are not well-defined. There are low levels of star formation.
