The galaxy presents an elongated, cigar-shaped morphology. Its central region displays a notably concentrated, bright, and reddish core. Extending outwards from the core, a fainter, bluish disk is visible. The disk appears relatively smooth. The galaxy exhibits no clear signs of spiral arm structure. The light distribution suggests the presence of both an older stellar population concentrated in the bulge and a younger stellar population in the disk. There are possible irregularities present within the disk.
