The galaxy presents as an elongated, lenticular or disk-like system, observed edge-on from our perspective. The central bulge appears prominent and moderately bright, exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk component is less defined, with diffuse light extending outwards from the bulge along the major axis. There are no apparent spiral arm structures or significant dust lanes visible in the image. The overall color gradient indicates a possible radial change in stellar population or dust content, with the outer regions of the disk appearing somewhat bluer. Based on its morphology and color, it appears to be a relatively massive galaxy, likely undergoing passive evolution. There is no obvious evidence of any recent or ongoing major merger events.
