The galaxy presents as a flattened, elliptical structure, highly inclined to our line of sight, appearing nearly edge-on. A bright, concentrated central bulge is observed, surrounded by a disk component. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. The disk displays a mottled texture with hints of spiral arm structure. The overall color gradient shifts from yellowish-white in the center to a bluer tint in the outer regions of the disk, indicative of a younger stellar population and ongoing star formation. There is evidence of dust lanes or dark obscurations within the disk, appearing as subtle, darker regions interspersed within the brighter areas. A faint halo is present, surrounding the disk, gradually fading into the background. The overall shape appears somewhat disturbed with a possible minor tidal interaction or past merger event.
