The galaxy presents as a somewhat smooth, elongated structure with a cigar-like shape. The light distribution appears relatively uniform, with a subtle concentration towards the central region. The color profile indicates a predominantly blue hue, suggesting the presence of a younger stellar population and ongoing star formation. There is little evidence of spiral arm structure or a prominent galactic bulge. No obvious signs of recent major mergers or significant tidal disturbances are visible. The galaxy is likely a disk galaxy viewed edge-on.
