The galaxy presents as a flattened, disk-shaped system, oriented edge-on relative to our line of sight. A prominent central bulge is evident, exhibiting a smooth, concentrated luminosity profile with a yellowish hue, suggesting an older stellar population. The disk component appears relatively thin and exhibits a reddish to yellowish color gradient outwards from the bulge, indicative of dust obscuration and potentially ongoing, albeit moderate, star formation. The overall morphology is suggestive of a late-type spiral or lenticular galaxy, however, the disk lacks any discernible spiral arm structure or distinct star-forming regions within this image. The galaxy is generally compact with smooth features.
