The galaxy presents as a relatively compact, elliptical-like structure. Its light profile appears smooth and centrally concentrated, lacking any discernible spiral arms or a prominent disk. The object's overall shape is somewhat elongated, showing a deviation from a perfectly circular morphology. There is a suggestion of some minor disturbances in its structure, possibly indicative of past interactions or minor merging activity. The galaxy exhibits a color profile that is slightly redder overall, suggesting an older stellar population and a reduced rate of ongoing star formation.
