The galaxy presents a flattened, elongated morphology, appearing as a lenticular or possibly a spiral galaxy viewed edge-on. Its central bulge exhibits a yellowish hue, suggestive of an older stellar population, likely dominated by red giant stars. The disk component shows a bluer tint, indicating the presence of younger, hotter stars and possibly some star-forming regions, although these regions are not clearly resolved in this image. There is an evident dust lane that causes a colour shift in the galaxy. The galaxy's overall structure appears relatively smooth and undisturbed, lacking prominent spiral arms or signs of a recent major merger event.
