The galaxy presents as an elongated, edge-on disk galaxy. A prominent central bulge dominates the morphology, appearing smooth and spheroidal with a concentration of yellow light indicative of an older stellar population. The disk component extends outwards from the bulge and is relatively thin. There is no clear presence of spiral arm structure or dust lanes visible in this image. The lack of distinct features suggests it is likely a quiescent galaxy with a low star formation rate. The color gradient from the central bulge outwards suggests a change in stellar population, with older stars concentrated in the bulge and younger stars possibly in the disk, although this is not clearly indicated in this image. There does not appear to be a significant tidal interaction or signs of an ongoing merger. The galaxy exhibits a smooth, undisturbed structure.
