The galaxy presents as a relatively smooth, disk-like structure viewed at an oblique angle. A central bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population with lower levels of ongoing star formation. The disk surrounding the bulge appears flatter, with a bluer color profile than the central region; hinting towards younger stars and potentially ongoing star formation. There is minimal evidence of spiral arm structure, but slight irregularities are present. The overall morphology appears relatively undisturbed, with no strong indications of a major merger event. Faint extensions are present on either side of the galaxy, but it is difficult to determine if these are tidal tails, or related to internal structure.
