The galaxy presents a largely smooth morphology, appearing somewhat elliptical in shape. The core exhibits a concentrated luminosity gradient, suggesting a significant stellar population density. A subtle color gradient is observed moving outward from the core, transitioning from a yellow-orange hue to a faint blue-green tint in the outer regions. This may indicate differing stellar populations and/or dust content.

The galaxy's structure appears relatively undisturbed, with no prominent tidal features or signs of major ongoing mergers visible. Slight asymmetry in the outer regions could hint at minor interactions or internal dynamical processes. Overall, the galaxy seems to be a relatively evolved system.
