The galaxy presents a generally smooth morphology, appearing as a centrally concentrated, elliptical-like object. There is a noticeable radial color gradient, transitioning from a brighter, yellower core to a dimmer, redder periphery. The absence of distinct spiral arms or prominent dust lanes suggests it is an early-type galaxy. The observed shape deviates slightly from a perfect circle, exhibiting a moderate degree of ellipticity. No obvious tidal features or signs of recent merger activity are discernible in the image, indicating a relatively undisturbed evolutionary history. The overall color profile suggests a stellar population dominated by older, redder stars, indicative of a low star formation rate.
