The galaxy presents as a relatively smooth, elliptical structure. There is a noticeable central bulge that appears yellowish in color, suggesting an older stellar population. The outer regions of the galaxy exhibit a bluer hue, which could indicate the presence of younger, hotter stars or ongoing star formation, albeit at a seemingly low rate. The overall morphology leans towards an elliptical shape, with a slight elongation. There is no clear evidence of spiral arms or a prominent disk structure. Minor disturbances may be present, though not enough to suggest an active merger event. The galaxy shows a high degree of central concentration.
