The galaxy presents as a relatively concentrated object. It displays a predominantly smooth, elliptical morphology, with no obvious spiral arm structures or a prominent disk component visible. Its overall shape appears somewhere between perfectly round and elongated, but close to round. The galaxy exhibits a yellow-red hue, which implies a population of older stars and a lower rate of current star formation activity. There is no strong evidence of a major ongoing merger event or significant tidal disturbances. Minor disturbances cannot be ruled out from the image alone. The galaxy shows a compact core. 
