The galaxy presents as a spindle-shaped object with a high degree of ellipticity, suggesting it is likely an edge-on disk galaxy. The color profile indicates a strong central concentration of older stars, exhibiting a yellowish-orange hue in the core. Moving outward from the center, the disk appears more diffuse. Some degree of dust lane obscuration may be present. The galaxy appears relatively isolated, lacking any prominent signs of ongoing major merger activity or strong tidal features. There is a slight asymmetry in the outer edges, indicative of minor disturbances or uneven gas distribution.
