This galaxy presents as an elongated disk, viewed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue which may suggest an older stellar population or significant dust obscuration. The disk component shows a bluer color, particularly at the edges, possibly indicative of recent or ongoing star formation. There is no obvious evidence of strong spiral arm structure, though the resolution limits precise morphological classification. The galaxy appears relatively undisturbed, lacking significant tidal features or indications of a major ongoing merger. The bulge appears to have a somewhat rounded morphology. There may be some faint dust lanes visible within the disk. 
