The galaxy presents as a relatively compact elliptical, exhibiting a smooth, featureless morphology. The central region displays a concentrated luminosity, indicating a possible dense stellar population or an active galactic nucleus. The color gradient transitions from a warmer, yellowish hue in the core to cooler, bluish tones in the outer regions, suggesting the presence of younger stars in the galactic halo, or perhaps a low level of on going star formation. There is no apparent spiral arm structure or significant dust lane obscuration. Minor asymmetry can be observed, suggesting a possible previous or ongoing minor interaction or disturbance, but this is not prominent. Overall, the galaxy appears to be an early-type system, likely with a substantial stellar mass.
