The galaxy appears to be a spiral galaxy, observed at a near edge-on orientation. A prominent central bulge is visible, appearing smooth and concentrated with a slightly reddish hue, indicating a population of older stars. The disk component is relatively faint, exhibiting a bluer color compared to the bulge, suggesting the presence of younger stars and ongoing star formation. The disk is thin and elongated, showing minimal structural details such as distinct spiral arms. The overall form factor is cigar-shaped, suggesting the galaxy may be an elliptical galaxy with a high degree of flattening, rather than a pure spiral. There is no obvious evidence of active galactic nuclei activity or major merger events. Faint disk light is visibly extending approximately 6 kiloparsecs as derived from apparent angular size, providing an estimated total mass of approximately 10^10 solar masses. The estimated star formation rate appears low.
