The galaxy presents an elongated, disk-like morphology, viewed at an oblique angle. A distinct central bulge is observed, exhibiting a yellowish-orange hue, which may indicate an older stellar population. The disk component displays a range of colors, transitioning from a similar yellowish-orange near the bulge to a bluer tint at the distal edges. This could indicate ongoing star formation regions present in the outer disk. There appears to be some form of disturbance in the morphology, with possible minor tidal tails or distortions in the disk. It's difficult to say for sure without more data.
