The galaxy presents a generally elliptical morphology, with a bright, concentrated central bulge region. The luminosity appears to decrease relatively smoothly with radial distance from the center. There's a slight elongation observed in the isophotes, suggesting it is not perfectly spherical, but has an aspect ratio somewhere between 0.7 and 0.9. The outer regions of the galaxy are significantly fainter than the core. A disk-like structure is not clearly visible. Given the colour profile, the galaxy appears to have a population of older stars dominating its light output, with fewer blue stars indicating relatively low current star formation. It appears mostly undisturbed, not showing distinct signs of recent or ongoing major merger events.
