The galaxy presents as a centrally concentrated elliptical morphology, generally smooth in appearance with a high degree of roundness. There is a strong central bulge, exhibiting a bright yellow-orange hue indicative of an older stellar population. The galaxy shows no obvious spiral arm structure or significant dust lanes. A subtle color gradient can be observed, with the central region appearing slightly yellower compared to the outer edges which seem a little redder. There's no obvious sign of any major mergers or tidal disturbances. The overall structure suggests a relatively evolved system, possibly with suppressed star formation activity.
