The galaxy presents as a spiral galaxy, viewed at a moderate inclination. Prominent spiral arms are visible, appearing somewhat flocculent in nature. Two main spiral arms are discernible, exhibiting a relatively tightly wound structure. The galaxy has a distinct central bulge, that takes up a significant portion of the galaxy's radius. The bulge is moderately sized and has a smooth texture. The spiral arms show a gradient in color, with bluer hues present at the outer edges, potentially indicative of ongoing star formation. A hint of a bar structure is present across the galaxy's central region. No major disturbances or signs of on-going merging are visible.
