The galaxy presents as an elongated, disk-shaped structure with a noticeable central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population dominating the core. The disk surrounding the bulge displays a bluer tint, indicative of ongoing star formation or a younger stellar population compared to the bulge. The galaxy appears relatively smooth with no prominent spiral arm structures immediately discernible; however, some subtle irregularities in the disk's brightness distribution hints at possible faint, tightly wound spiral arms. The overall shape is highly elongated, almost cigar-shaped, implying that we may be viewing the galaxy close to edge-on. No significant tidal disturbances or interactions with neighboring galaxies are apparent in this image.