The galaxy presents as a prominent, elongated object, indicative of a disk galaxy viewed nearly edge-on. A central bulge is visible, appearing to be primarily composed of older stellar populations, inferred from its yellowish-orange hue. The bulge has a somewhat rounded profile. The disk appears relatively smooth, with limited discernible substructure such as spiral arms or prominent dust lanes. The disk itself appears to be exhibiting some ongoing star formation, as suggested by the bluer component extending along its length. Overall, the galaxy appears undisturbed, with no signs of major mergers or tidal interactions. The estimated size suggests it is a relatively large galaxy.
