The observed galaxy presents as a single, relatively compact object. Its morphology appears smooth and largely featureless with an approximate circular shape, showing minimal signs of disk-like structures or spiral arms. There is a slightly elongated quality to the shape, but not significantly. The overall light distribution is concentrated toward the center, gradually decreasing outwards. The galaxy appears to have no distinct nucleus or core region. There are no indications of significant ongoing merger activity or major disturbances to the galaxy's overall structure. The lack of resolved features suggests this is likely an elliptical galaxy.
