The galaxy presents as a centrally concentrated, elliptical-like structure. Its morphology appears smooth and largely featureless upon visual inspection, with a high degree of central concentration. The color profile indicates a yellowish core, suggesting an older stellar population dominates the central regions. Fainter blueish hues extend outwards from this core, tracing what may be regions of more recent star formation. There appears to be little evidence of spiral arms or significant dust lanes; there are no obvious signs of ongoing or recent major mergers and only minor distortions seem to be present. The overall roundness of the object indicates a relative lack of flattening. The galaxy does not exhibit a highly active star-forming nature.
