The galaxy presents as a flattened, elliptical morphology. The central region exhibits a concentrated, bright luminosity, transitioning outward to a diffuse halo. The color profile shifts from a predominantly red-yellow core to a subtle blue-green tinge at the periphery. The overall structure appears relatively undisturbed, with no prominent tidal features or signs of major mergers visible. The observed shape is elongated, with the major axis significantly larger than the minor axis, suggesting a high inclination angle relative to the observer's line of sight. The smoothness of the light distribution is evident, with a lack of distinct spiral arms or clumpy star-forming regions. Based on these observations, the galaxy is likely a relatively massive early-type system exhibiting low levels of star formation.
