The galaxy presents a largely smooth and elliptical morphology, with a high degree of central concentration indicated by the bright, yellowish-orange core. A very faint, diffuse halo surrounds this core, exhibiting a gradual decrease in luminosity with increasing radial distance. There is little evidence of distinct spiral arm structures or significant dust lanes, suggesting the object is a relatively evolved system with a low current rate of star formation. The galaxy appears generally rounded, with no obvious signs of major tidal disruption or interaction, although there is a hint of a minor disturbance or faint feature extending from one side of the galaxy. The overall color profile suggests a stellar population dominated by older, redder stars.
