The galaxy presents as a relatively small, disk-shaped structure. It exhibits a noticeable central bulge that appears bright and yellowish in color, suggesting an older stellar population. The disk component is not well-resolved, but seems to be oriented close to edge-on from our perspective. The disk itself appears smoother in texture than the bulge, and shows signs of blue light, hinting at ongoing star formation. There are no readily apparent spiral arms or bar structure. Overall, the morphology suggests a galaxy that may be transitioning towards a more quiescent state, with the bulge dominating the light output.
