The galaxy presents as a centrally concentrated object with a generally smooth morphology. It appears approximately circular. The central region exhibits a bright, relatively compact core. The light profile gradually decreases outward from the core, with a diffuse halo surrounding the central brightness. There is minimal evidence of spiral arm structure or distinct features in the disk, suggesting either a lack of prominent spiral arms or a near face-on orientation. A slight asymmetry is observed, possibly indicating a minor gravitational disturbance. The color profile seems relatively uniform across the galaxy, leaning towards bluer hues in the central region.