The galaxy presents a largely smooth, elliptical morphology, with an estimated effective radius suggesting a moderately sized system. Its color profile indicates a predominantly older stellar population, with a central region exhibiting a yellow-orange hue that fades gradually towards the outer edges. There is a subtle indication of blue light present in the galaxy. The galaxy is mostly smooth with no real indication of distinct structural features or prominent spiral arms. It appears relatively undisturbed, showing no significant signs of ongoing mergers or tidal interactions. 
