The galaxy appears as a relatively smooth, centrally concentrated object. It displays an elliptical morphology, with a gradual falloff in surface brightness from the core outwards. The color profile suggests a predominantly older stellar population. The core exhibits a yellow to orange hue, indicative of evolved stars, potentially including red giants and supergiants. There is a subtle color gradient towards the outer regions, with hints of bluer tones, although the prominence of blue light is not significant, suggesting a relatively low rate of ongoing star formation. No distinct spiral arms or prominent dust lanes are apparent. There is no evidence of strong tidal features or other indicators of recent major merger activity. The galaxy presents a fairly undisturbed and relaxed appearance. Overall, the galaxy is likely a massive early-type galaxy exhibiting properties consistent with a quiescent stellar population.
