The galaxy presents as an elliptical morphology, with a relatively smooth, centralized luminosity profile. The central bulge exhibits a strong concentration of light, transitioning into a fainter, less defined halo. The galaxy appears to be an intermediate elliptical type, somewhere between perfectly spherical and a more elongated, cigar-like shape. There is no discernible spiral structure or evidence of significant dust lanes. The overall color profile suggests an older stellar population, with a reddish hue dominating the central region. There is no obvious indication of major mergers or tidal disturbances affecting the galaxy's structure, although minor disturbances cannot be completely ruled out.
