The galaxy presents as a spiral type with a centrally concentrated bulge. The color gradients suggest a bulge comprised of older stellar populations exhibiting a yellowish-orange hue. Spiral arms are visible, though somewhat diffuse. These arms appear to have a medium winding, tracing outwards from the central bulge. There is evidence of active star formation within these arms, indicated by the presence of bluer regions. Two prominent arms are visually distinguishable. The galaxy shows no obvious signs of major tidal disturbances indicative of an ongoing or recent major merger event, though minor irregularities cannot be entirely ruled out. The disk is not viewed edge-on, instead seen at a fairly face-on angle allowing for spiral arm structure observation. A faint bar-like structure may be present, bisecting the bulge region, though it is not a very prominent feature. The bulge itself appears to be a moderate size in comparison to the disk.
