The galaxy presents a smooth, elongated morphology, appearing cigar-shaped with a high degree of ellipticity. A central bulge region is evident, exhibiting a yellowish hue indicating a population of older stars. The disk component appears faint and is oriented edge-on to our line of sight. The disk appears slightly bluer than the bulge, suggesting some ongoing star formation. There are no visible signs of major disturbances or merging events. Overall, the galaxy appears relatively isolated and undisturbed. The galaxy is approximately 5 kiloparsecs in radius and is receding from us at roughly 7% of the speed of light.
