The galaxy presents as a relatively smooth and elongated structure. The central region exhibits a higher concentration of light, suggesting a bulge or core component. The overall color profile appears redder in the central regions, transitioning towards bluer hues in the outer regions. This color gradient could indicate variations in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars in the outer regions. The shape is distinctly cigar-shaped, exhibiting a high degree of ellipticity. There is no clear indication of prominent spiral arms or significant dust lanes. No major signs of ongoing merger events or tidal disruptions are observed, although subtle disturbances cannot be ruled out. The galaxy shows an estimated mass of 10^10 solar masses and a moderate amount of star formation.
