The galaxy presents as a moderately inclined disk galaxy. A central bulge component is visible, appearing roughly spherical and exhibiting a yellowish hue, suggestive of an older stellar population. The disk surrounding the bulge is predominantly blue, indicative of ongoing star formation. The galaxy appears to be relatively undisturbed, with no clear signs of recent major mergers or tidal interactions.  There is some indication of minor disturbances. The spiral arms are not particularly well-defined, contributing to a somewhat flocculent appearance. The light distribution suggests a moderate mass.
