The galaxy appears as a faint, elongated structure with a relatively smooth overall morphology. There is a subtle colour gradient across the galaxy, with the central region exhibiting a slightly redder hue than the outer edges, hinting at a possible older stellar population towards the center. The galaxy is small and somewhat cigar-shaped, with no clear evidence of spiral arms or a prominent disk. There is some minor clumping within the galaxy's structure, possibly indicating regions of ongoing, but not exceptionally high, star formation. No obvious signs of a major merger are immediately apparent, but the structure displays hints of minor disturbances.
