The galaxy presents as a relatively smooth, elongated structure. Its overall shape is reminiscent of a cigar, with a high axis ratio suggesting an elliptical morphology viewed at an oblique angle or a highly inclined spiral galaxy. The color profile exhibits a central region dominated by yellowish-orange hues, indicative of an older stellar population with lower levels of recent star formation. There is a faint hint of bluer emissions on the edges of the disk, which suggests on-going star formation, however it is not pronounced. There is no obvious presence of distinct spiral arms, bars, or strong tidal features, the galaxy appears isolated and well-formed. The smooth light distribution implies a well-mixed stellar population with no major merger events disturbing its symmetry. The galaxy is small but distinct, having an apparent size on the order of a few arcseconds. Overall, the galaxy's morphology aligns with that of an elliptical galaxy or a lenticular galaxy seen edge-on, with a notable lack of prominent features suggesting low ongoing star formation.
