The galaxy presents as a somewhat elongated, disk-like structure, with a smooth overall appearance. The central region displays a concentration of light, suggestive of a bulge, that seems to fade outwards. The galaxy appears to be tilted relative to our line of sight.

The color distribution across the galaxy is not uniform. The central bulge appears to be more red/yellow in color, possibly indicating an older stellar population or a higher concentration of dust. Fainter, blueish regions are visible on the outer edges of the disk, suggesting the presence of younger, hotter stars. A small knot of bluer light is visible on one side of the disk, which could indicate an area of active star formation. There is no indication of strong spiral arms.

There seems to be very minor disturbance in the morphology, with some light appearing slightly asymmetrical. I do not see any evidence of a major merger event.
