The galaxy presents a primarily smooth and elliptical morphology. The core exhibits a bright, concentrated luminosity, suggestive of a significant stellar density, possibly indicating an older stellar population. The surrounding halo displays a gradual decline in luminosity, with a color gradient shifting from a yellowish-white core to a more reddish hue in the outer regions. This color variation may be indicative of varying stellar populations and star formation histories across the galaxy, with the redder outer regions potentially hosting older, less massive stars. No distinct spiral arms or dust lanes are visible, contributing to its overall smooth appearance. There appears to be no strong evidence of a major ongoing merger or significant tidal disturbances.
