The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellow-orange hue, suggestive of an older stellar population. The outer regions appear less defined, gradually fading into the background sky. There is a subtle color gradient from the core outwards, with the outer regions appearing slightly bluer, implying the presence of a younger stellar population, but this is very slight. Overall, the galaxy shows no significant signs of spiral arms or major disturbances. The high degree of roundness suggests a classification closer to E0-E3 on the Hubble sequence.
