The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, with a noticeable radial color gradient, transitioning from a yellow-orange core to a dimmer, reddish-orange periphery. The core appears to be dominated by older stellar populations, as evidenced by the yellow hue, suggesting a lack of significant recent star formation in that region. No distinct spiral arms or prominent dust lanes are discernible. There is a subtle suggestion of tidal features or minor disturbances, but not enough to categorize it as actively merging. The galaxy appears quite massive, and its overall morphology suggests it is a relatively evolved system.
