The galaxy appears to be a spiral galaxy viewed edge-on or at a high inclination. The central bulge is quite prominent and has a yellowish-orange hue, suggesting a population of older stars. A faint, blueish disk extends outwards from the bulge on either side. The blue color indicates the presence of younger, hotter stars, and potentially ongoing star formation within the disk. There may be a faint dust lane visible along the midplane, further indicative of a spiral structure. Some slight distortions are also visible, which could be the result of past or ongoing interaction.
