The galaxy presents as a relatively smooth, elliptical-like structure. It has a bright central bulge that gently fades into the outer regions. There is a slight indication of a disk. No prominent spiral arms are visible. Color gradients suggest a mature stellar population, with a higher concentration of older, redder stars in the central regions. There is no strong evidence of active star formation regions. No tidal tails or morphological disturbances suggest past or ongoing mergers.