The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth morphology. There is a slight elongation, suggesting a deviation from a perfectly spherical shape, but overall it presents a rounded form. The galaxy's core is characterized by high luminosity, which gradually diminishes towards the outer regions. The color profile is broadly consistent, leaning towards warmer tones, indicative of an older stellar population with lower levels of ongoing star formation. There's no apparent spiral arm structure or significant dust lanes visible in this image. The overall structure suggests the galaxy is relatively undisturbed, without obvious signs of a recent major merger event.
