The galaxy presents as a disk galaxy, observed nearly edge-on from our line of sight. A central bulge, characterized by a concentrated, yellowish-orange hue, dominates the structure. The bulge appears relatively smooth, with no discernible substructure. Fainter, bluish light extends outward from the bulge, tracing the galactic disk. The disk is thin and elongated, with a hint of dust lane obscuration. No distinct spiral arm structure or prominent star-forming regions are apparent in the image. The galaxy shows no clear signs of a recent or ongoing major merger event, although a slight asymmetry cannot be ruled out. The rounded shape of the bulge is typical of disk galaxies, suggesting it is not the product of a recent merger. The lack of strong blue emission in the disk is suggestive of a relatively low star formation rate, and thus a population of older stars.
