The galaxy presents a generally elliptical morphology. The central region exhibits a bright, concentrated core with a yellowish-white color, suggesting a population of older stars. Moving outwards from the core, the color grades to a more diffuse, reddish hue in the outer regions. This color gradient likely indicates a decline in the average stellar age as well as lower metallicity and/or dust extinction in these outer areas. There are no obvious spiral arm structures, but a very faint disk may be present. The galaxy does not show any signs of ongoing major mergers or significant tidal disturbances in this image.
