The galaxy presents as a relatively smooth, elliptical form. Its core exhibits a concentrated, bright yellow hue, suggesting a population of older stars. A gradual decline in luminosity extends outwards from the core. A faint greenish tint encircles the core, possibly indicating some ongoing, albeit limited, star formation. There is no clear disk structure and no evident spiral arm morphology. The general symmetric form and lack of significant disturbances suggest that it is a relaxed system, not undergoing any major mergers at the present time.
