The galaxy presents as a relatively smooth, elliptical morphology. Its color profile appears to be generally redder, suggesting an older stellar population with lower rates of ongoing star formation. The galaxy exhibits a centrally concentrated luminosity profile, consistent with a bulge-dominated system. There is no apparent spiral arm structure or significant dust lane obscuration visible in the image. The galaxy appears relatively undisturbed, showing no strong signs of recent merger activity. The shape is quite circular. The galaxy is relatively large and quite bright.
