The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. It exhibits a bright, yellowish core region that diffuses outward. There's a noticeable lack of distinct spiral arms or prominent dust lanes, reinforcing the assessment of a primarily smooth morphology. The galaxy appears to be generally undisturbed, with no evident signs of major mergers or significant tidal distortions. Overall, the galaxy presents a somewhat spheroidal appearance, with a gradual transition in brightness from its center to the outer regions. The color profile suggests an older stellar population dominating the light emission.
