The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. Its overall shape is somewhat elongated, presenting a flattened appearance. The color profile indicates a general yellowish-white hue, with a slightly redder tint in certain regions. While no distinct spiral arm structures are evident, subtle variations in color and brightness suggest the presence of underlying features, possibly related to dust lanes or regions of star formation activity. There are some minor disturbances, suggesting the potential for some kind of interaction. These are not major disruptions and the overall mass estimate would be somewhere between 10 to the 10th and 10 to the 11th solar masses. From our vantage point, the galaxy seems to be transitioning from a more active star-forming phase to one with suppressed or quenched activity.
