The galaxy appears as a centrally concentrated object with an overall elliptical morphology. Its core exhibits a bright, yellowish-white hue, suggesting an older stellar population with a lower rate of star formation. The galaxy's overall shape is elongated, but it's neither perfectly round nor distinctly cigar-shaped. There is a slight hint of asymmetry or a minor disturbance present, but the galaxy is not exhibiting strong signs of a major merger event. Faint blue edges can be observed along the more distant edges of the galaxy, potentially indicating a slightly higher amount of star formation than the galaxy's core. The system does not exhibit a pronounced disk structure or spiral arms.
