The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellowish hue, suggestive of an older stellar population. The surrounding halo is less defined, fading into a darker, bluer color, which may indicate a sparse distribution of younger stars or a lower overall stellar density. There are no apparent spiral arm structures or prominent dust lanes visible in this image. The galaxy appears to be relatively isolated, showing no signs of ongoing or recent major merger events, though the presence of a minor disturbance cannot be ruled out. Overall, the galaxy's light profile indicates a relatively evolved system.
