The galaxy appears as a moderately luminous object exhibiting a flattened, somewhat elongated shape. The light distribution appears relatively smooth and centrally concentrated. No distinct spiral arms or a prominent bulge is visible. The galaxy's color is slightly yellowish suggesting an older stellar population. The morphological analysis suggests this galaxy might be a disk galaxy. Some minor disturbance in its shape is noticeable. There are no other indications of recent or ongoing major mergers or interactions.
