The galaxy presents as an edge-on or highly inclined disk galaxy. A prominent central bulge is visible, appearing somewhat elliptical and displaying a yellowish hue, suggesting an older stellar population. The disk component is flattened and exhibits a bluer color gradient extending outwards from the bulge, consistent with younger stars and potential star-forming regions. There's a degree of asymmetry within the disk, with a slight warp or irregularity noted. Faint, diffuse material extends beyond the primary disk structure, possibly indicative of a stellar halo or tidal features resulting from past interactions. The galaxy does not appear to be undergoing a major merger, but there could be minor disturbances present based on the disk shape and presence of extended material. Overall, the galaxy presents as a relatively massive system with a low star formation rate.
