The galaxy presents as a primarily smooth, elongated structure. A central bulge dominates the galaxy's luminosity, displaying a yellowish-orange hue. Fainter, bluer light extends outward from the bulge along the major axis, suggesting the presence of a disk component seen nearly edge-on. The disk appears relatively undisturbed, exhibiting only minor irregularities in its overall form. There is no strong evidence of active merging or significant tidal features. The galaxy's color profile indicates a potential mix of older stellar populations concentrated in the bulge and younger populations within the disk. Overall, the galaxy appears as an early type spiral, nearly edge-on.
