The galaxy presents as a smooth, centrally concentrated object with a generally elliptical morphology. The light distribution appears relatively uniform, lacking prominent spiral arm structures or significant dust lane features. A colour gradient is observed, with the central region exhibiting a yellowish hue, transitioning to a slightly redder colour towards the outer edges. This suggests an older stellar population concentrated at the centre. There is no apparent evidence of ongoing major mergers or significant tidal disturbances.
