The galaxy presents as a relatively smooth, elliptical morphology. The core region exhibits a bright, concentrated luminosity, with a noticeable color gradient shifting towards redder hues. This indicates a potentially older stellar population dominating the central region, possibly with suppressed levels of recent star formation. There is a gradual decrease in luminosity moving outward from the core, exhibiting an absence of prominent spiral arms or distinct features. The overall structure suggests the galaxy is in a relatively quiescent state, showing no obvious signs of major mergers or significant disturbances in its morphology. It is slightly oblong in shape and fairly homogenous in its structure.
