The galaxy exhibits a central bulge that appears relatively smooth and concentrated. Extending outward from the core, there is a fainter disk component. The galaxy does not display a highly defined spiral structure, but some patchy, irregular features can be observed suggesting some non uniformity in the disk. The overall color profile indicates a mix of stellar populations, with bluer hues in certain regions of the disk that could indicate ongoing star formation activity. There also appear to be some disturbances, possibly due to interactions with a nearby galaxy.
