The galaxy presents as a centrally concentrated, elliptical structure with a smooth light distribution. The core region is bright and gradually fades outwards, exhibiting a radial decrease in surface brightness. The galaxy appears to be a spheroid with a very minimal disk component. There is no visual evidence of spiral arms or significant dust lanes. Based on the color profile, the object exhibits a redder hue, suggesting an older stellar population. There is no visually apparent signs of tidal disturbances or ongoing major mergers. The morphology appears undisturbed, indicative of a relaxed or quiescent galaxy state.
