The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse light distribution. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. There is a subtle color gradient observed from the center outwards, transitioning towards a redder, less luminous halo. No distinct spiral arms or prominent dust lanes are visible. There is a slight elongation, indicating that it is likely not perfectly spherical. There are no signs of on-going major merging activity or tidal disturbances, suggesting it is in a relatively quiescent state. Star formation appears to be weak, as evidenced by the absence of strong blue colors typically associated with young, hot stars.
