The galaxy presents a largely smooth, elliptical morphology. It displays a concentrated central bulge, characterized by a yellowish hue suggestive of an older stellar population. The overall shape is somewhat elongated, but not markedly so. There is no apparent disk structure, or spiral arm presence. Subtle irregularities hint at the possibility of minor disturbances in the galaxy's structure, but no major mergers or significant tidal features are apparent. The color gradient suggests a slight reddening towards the core, potentially indicative of higher dust concentration or a more metal-rich stellar population in that region. The galaxy's luminosity is suggestive of a massive system.
