The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a distinct core region exhibiting a yellowish hue, suggesting a significant population of older stars. The light gradually diminishes with increasing radius, transitioning into a more diffuse outer halo. No distinct spiral arm structures or dust lanes are discernible within the observed image. The overall appearance indicates a relatively evolved system with little evidence of ongoing major star formation activity. There is a subtle, but apparent, flattening in the galaxy's shape, suggesting it is not perfectly spherical. There is a faint hint of bluer light in the outskirts of the halo, suggesting that there may be small pockets of ongoing star formation. The structure is seemingly undisturbed with no obvious signs of ongoing or recent merger events.
