The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light distribution. The central region displays a concentration of light, appearing yellowish-white, indicative of an older stellar population. Moving outward from the core, the light fades into a bluish hue, though the overall color remains relatively uniform, suggesting a lack of significant dust lanes or active star-forming regions throughout. The galaxy does not display any apparent spiral arm structure or other distinct features usually associated with disk galaxies, like ongoing merging activity. Overall, it presents as a moderately luminous galaxy.
