The galaxy appears to be a relatively smooth, elliptical system. Its light profile suggests a centrally concentrated morphology, with a gradual decrease in luminosity towards the outer regions. There is little evidence of spiral arms or significant dust lanes. The galaxy exhibits a yellowish-red hue, which would indicate an older stellar population and minimal ongoing star formation. Its overall shape is neither perfectly spherical nor highly elongated, but appears to be in between. No signs of significant tidal disturbances or ongoing mergers are visible.