The galaxy presents an elongated, cigar-shaped morphology with a prominent central bulge. Its overall color profile appears to be primarily bluish-white, suggesting a stellar population with a significant proportion of younger, hotter stars. The galaxy's disk is viewed nearly edge-on, and is smooth in texture. The central bulge exhibits a more concentrated luminosity, which gradually fades outward along the length of the disk. Evidence of internal spiral structures or prominent dust lanes is not visible. Faint traces of bluer luminosity extend away from the main body of the galaxy, possibly indicative of tidal features or extended stellar halos.
