The galaxy appears to be a relatively undisturbed, disk-shaped object, viewed at a moderate inclination angle. It is likely a spiral galaxy as indicated by it's morphology, though definitive spiral arm structure is not apparent in this image. The central bulge region exhibits a yellow-orange hue, suggesting an older stellar population. A faint, flattened disk extends outwards from the bulge. There might be the suggestion of a bar feature crossing the nuclear bulge, but its presence is not conclusive. The colours become slightly bluer towards the outer edges of the disk, potentially indicating the presence of younger, hotter stars and some ongoing star formation in these regions. The galaxy is moderately luminous and of intermediate mass, with a measured redshift.
