The galaxy presents as a somewhat elongated structure. Its morphology appears to be largely smooth with an indication of a disk like component. There's a relatively bright, central bulge that is slightly offset from the main axis of the galaxy, which gradually fades towards the outer edges. The color gradient shifts from warmer hues in the center to cooler tones further out, suggesting variations in stellar populations or dust content across the galactic disc. It's strongly cigar shaped. There are no obvious signs of major tidal disturbances or ongoing mergers, but there are indications of minor disturbances.
