The galaxy presents as a spiral type, exhibiting a moderately sized central bulge. The spiral arms are clearly defined and appear to be wound relatively tightly. A central bar structure is present, extending through the bulge region. The overall disk appears disturbed, possibly due to gravitational interactions or ongoing merger activity. Light from the bulge is yellowish, with bluer light emanating from the spiral arms. The disk appears to be inclined at a slight angle relative to our line of sight.
