The galaxy presents as a spiral system exhibiting significant disturbances, potentially indicative of an ongoing or recent merger event. The central bulge is moderately sized and appears yellowish, suggesting an older stellar population. Faint spiral arms extend from the bulge, displaying a winding pattern of medium tightness. They appear to be somewhat amorphous and show irregularities, further supporting the presence of gravitational interaction. The galaxy's overall shape is elliptical.
