This galaxy presents as an elongated, disk-shaped structure, oriented nearly edge-on relative to our line of sight. The central region exhibits a higher surface brightness and a yellowish-white hue, suggestive of an older stellar population or dust obscuration. Extending outward from the core, bluer colors dominate, indicating the presence of younger, hotter stars and ongoing star formation within the galactic disk. The disk appears relatively smooth, lacking prominent spiral arm structures or strong irregularities. There is some subtle clumping of stars, perhaps faint spiral arms in the disk region. The overall morphology suggests a relatively quiescent state, though the bluer periphery indicates active star formation. There is no apparent tidal distortion or major morphological disturbance, suggesting it is relatively isolated, though a very close inspection may show minor disturbances.
