The galaxy presents as a largely smooth, centrally concentrated object with an elliptical morphology. The light profile appears to be dominated by an extended, diffuse spheroid component, lacking any prominent spiral arm structures or a well-defined disk. The central region exhibits a brighter, more concentrated luminosity, potentially indicative of an active galactic nucleus or a dense stellar population within the galactic core. There is subtle colour variation in the image, with a tendency towards slightly bluer hues in the outer regions relative to the more reddish central bulge. This may suggest a differential stellar population, with younger, hotter stars residing further from the core, and older, cooler stars concentrated towards the center. There is a slight asymmetry in the luminosity distribution, but no clear evidence of tidal streams or ongoing major merger events. Overall, the galaxy appears to be a relatively evolved system, potentially undergoing a period of quiescent star formation.
