The observed galaxy presents as a spiral galaxy, viewed at a slight angle. The spiral arms are well-defined and extend outwards from a central bulge. There is evidence of a strong bar structure crossing the galactic center, which is oriented nearly horizontally in the image. Dust lanes are visible along the inner edges of the spiral arms. The bulge appears yellow, suggesting an older stellar population. The spiral arms show regions of blue light, indicative of active star formation. The winding of the spiral arms appears tight, tightly wrapped around the galaxy. The galaxy shows no signs of significant disturbances or interactions with other galaxies, indicating that it has not merged with another object recently. There is no other object merging with it and there are no major tidal features.
