The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The light distribution appears largely uniform, suggesting a well-mixed stellar population. The overall color is slightly yellowish-orange, potentially indicating a population of older, cooler stars with lower levels of on-going star formation. There is a subtle suggestion of a diffuse halo surrounding the core region. The galaxy does not exhibit any obvious signs of spiral arms, strong dust lanes, or other distinct features indicative of active star formation or recent mergers.
