The galaxy presents as an elongated, cigar-shaped structure. There appears to be a relatively smooth central bulge with a concentration of light. Extending outwards from this central region, the galaxy exhibits a disk-like structure. The disk appears highly inclined to our line of sight. There seems to be a color gradient visible, with the central bulge exhibiting a redder hue compared to the outer regions of the disk. The galaxy displays indications of a spheroidal structure, although this is hard to confirm due to image quality. Overall, the galaxy exhibits a disturbed morphology, with the potential for tidal effects or interaction.
