The galaxy presents an overall elongated, cigar-shaped morphology. Its central region exhibits a brighter, more concentrated luminosity, suggestive of a galactic nucleus or bulge. The light gradually diffuses outwards from the core, with some areas appearing fainter and bluer. This implies an older stellar population concentrated in the center and younger stars in a possible, somewhat indistinct disk structure. There are no clear spiral arm structures visible, but minor tidal disturbances might exist. There are no signs of a recent major merger event. The shape appears to be relatively smooth. 
