The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is a slight elongation, indicating a shape that deviates from perfectly spherical. The color gradient suggests a yellow-white core, transitioning to redder hues in the outer regions. The overall color profile indicates an older stellar population. The light is fairly evenly distributed, with no distinct spiral arm structures or prominent dust lanes visible. There is some possible disruption in the bottom central section, possibly indicating a feature or disturbance.
