The galaxy presents as a spiral galaxy with a moderately sized bulge. The spiral arms are well-defined and exhibit a tightly wound morphology. They appear somewhat patchy in color, with regions of bluer light likely indicating areas of active star formation. The central bulge shows a yellowish hue, consistent with an older stellar population. The disk appears relatively smooth, with no major disturbances readily apparent. The galaxy is viewed at a slight angle relative to edge-on. A faint bar structure may be present, as hinted by a slight elongation of the central region. There is no obvious evidence of a major merger event, although a minor interaction cannot be ruled out.
