This galaxy presents a predominantly smooth morphology. The central region exhibits a high surface brightness, indicative of a dense stellar population, potentially an aging population. The galaxy appears moderately elliptical, with an axial ratio suggesting a shape somewhere between circular and elongated. There's a suggestion of faint, diffuse extended emission surrounding the core, transitioning into the background sky. There are no obvious spiral arm structures or distinct dust lanes visible in this image, furthering the impression of a relatively undisturbed system. Overall, the galaxy’s structure is consistent with an elliptical or S0 galaxy at moderate redshift.
