The galaxy appears to be a relatively compact system. Its light profile is smooth and centrally concentrated. The central region appears to be dominated by an older stellar population with some indication of ongoing star formation. The galaxy exhibits a morphology that is neither fully elliptical nor spiral, appearing to be disk-like but relatively featureless. There are subtle hints of a disk structure, however, there is no presence of well-defined spiral arms or a prominent bulge. There is potential evidence of some minor disturbance or interaction, as there are slight irregular features.
