The galaxy presents as a spiral galaxy, viewed at an oblique angle, but not quite edge-on. There is a central bulge region with an elongated, bar-like structure extending through it. The spiral arms are evident, though somewhat tightly wound. They appear asymmetric, with one arm appearing more defined than the other. There is a clear color gradient, with the bulge exhibiting a yellow hue indicative of an older stellar population, whereas the outer spiral arms suggest bluer, younger stars. There may be some minor disturbances suggesting a possible interaction or merging event. There's likely low current star formation overall, but the spiral arms still show some indications of it. The galaxy's overall morphology suggests it could be a barred spiral.
