The galaxy presents as a disk galaxy, viewed at an oblique angle. A prominent central bulge is visible, exhibiting a yellowish hue, possibly indicative of an older stellar population. Extending from the bulge is a disk, less defined, but discernable. The disk presents with a bluer color than the central bulge, hinting at ongoing star formation. The overall form suggests a spiral, albeit one with less pronounced or tightly wound spiral arms. There is a faint luminous object in close proximity to the main galactic body, this may indicate a minor interaction or merger event. Overall, the galaxy does not appear to be strongly disturbed.
