The galaxy presents as a single, diffuse object, without a well-defined spiral structure. The light is concentrated primarily in the central region, with a noticeable decrease in surface brightness towards the outer regions. There's a slight asymmetry, suggestive of potential tidal interactions or an irregular morphology. The overall color appears to be intermediate, hinting at a mixed stellar population, possibly with both older and younger stars contributing to the observed light. The lack of distinct spiral arms or prominent dust lanes suggests a relatively quiescent or possibly post-merger state. There are some indications of disturbance to its shape, perhaps it is in a close encounter with a nearby galaxy. 
