The galaxy presents as a relatively smooth, elliptical-type structure. It exhibits a concentrated central region, with a gradual decrease in luminosity towards its outer edges. The galaxy's color profile appears to be dominated by yellowish hues, suggesting an older stellar population and relatively low rates of ongoing star formation. The shape is generally rounded with a slight elongation, not quite a perfect sphere. There is no distinct disk component visible, nor is there evidence of spiral arms or prominent dust lanes. No signs of any major ongoing merger events are apparent in the image, though there might be minor disturbances to the structure.
