The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. It has an overall yellowish-red hue suggesting an older stellar population and a relatively low rate of star formation. The object is elongated, with the shape being somewhat cigar-like, but mostly in between round and elongated. There appears to be little evidence of spiral arms or disk structures, further supporting its classification as an elliptical galaxy. The overall structure seems undisturbed, and there are no clear signs of ongoing or recent major merger events. The redder colors toward the center suggest a higher concentration of older stars, while slightly bluer hues towards the outer edges might indicate some residual star formation.
