The galaxy presents as a centrally concentrated object with a relatively smooth morphology. The light distribution appears elliptical, exhibiting a high degree of roundness. There is no clear evidence of spiral arms or a prominent disk structure. The color profile suggests a dominant older stellar population, with a reddish-yellow hue concentrated in the central region, fading to a more blueish color towards the edges. There is a slight asymmetry to the galaxy, but the overall structure appears mostly undisturbed. Overall, the galaxy is relatively compact.
