The galaxy presents a generally smooth morphology with a high degree of roundness. There is some evidence of subtle structural features or a disk, but overall it appears largely featureless. The color profile indicates a centrally concentrated, older stellar population likely dominating the light output, evidenced by the redder hue at its core. Outer regions show bluer colors, perhaps indicating some star formation activity. There are no readily apparent signs of major mergers or significant tidal disturbances. The galaxy appears relatively isolated and relaxed in its morphology.
