The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears spheroidal and dominates the overall light profile. Moving outward from the bulge, the light gradually diffuses, showing a smooth decline in surface brightness towards the edges. There is minimal evidence of spiral arm structures or significant dust lanes in the image. The galaxy possesses a yellowish-red color, suggesting an older stellar population, potentially with limited ongoing star formation. It does not appear to be undergoing any major merger events or significant tidal distortions. There might be a very subtle disk component as the shape deviates slightly from perfectly circular, although further observations at higher resolution may be necessary to confirm this.
