The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It appears to exhibit a moderate degree of roundness but may be better described as "in between" round and elongated. There is a faint blue-ish hue surrounding the central core that fades into the surrounding dark sky, suggesting the presence of some star formation activity. The lack of defined spiral arms or obvious dust lanes implies a relatively evolved system, likely with a stellar population dominated by older stars. The overall morphology suggests a galaxy that has potentially undergone some minor disturbances, although no major merger events are immediately apparent. The galaxy is a decent distance away, making it less clear than the foreground elements that can be seen around it. 
