The galaxy presents a generally smooth morphology, with a slight elongation but is mostly rounded in shape. There is a hint of a disk structure, but it is not sharply defined; rather, it appears somewhat diffuse. The galaxy's core exhibits a higher concentration of light, fading towards its outer regions. The object displays characteristics of both an elliptical and a spiral galaxy, with a prominent bulge region and subtle disk features.

The color profile suggests a population of older stars, as it appears redder than bluer. No prominent dust lanes or distinct spiral arms are visible in this imaging, indicating a relatively quiescent stage of star formation. There may be a small merger happening in the galaxy, or perhaps a minor disturbance as the shape seems slightly off. 
