The galaxy exhibits a generally smooth morphology, suggesting an elliptical or lenticular type. The light distribution appears centrally concentrated with a gradual decrease in brightness towards the outer regions. The shape is somewhat elongated, but overall fairly rounded. The central region displays a yellowish hue, potentially indicating a population of older stars. There are no obvious spiral arms or significant dust lanes visible. No major signs of tidal disturbances or ongoing mergers are readily apparent.
