The galaxy appears to be a spiral galaxy, viewed at an oblique angle relative to its plane. A central bulge is clearly visible, exhibiting a yellowish hue, suggestive of an older stellar population. The disk component surrounds the bulge and displays hints of spiral arm structure, though the resolution is insufficient to discern distinct, well-defined arms. The disk shows a bluer color, indicative of ongoing star formation within the spiral arms. The galaxy's overall shape is elongated, consistent with a spiral galaxy seen at an angle. There are no obvious signs of significant tidal disturbances or ongoing mergers. The galaxy presents as a relatively undisturbed system, displaying a classic spiral morphology.
