The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a concentrated, bright yellowish-orange hue, which gradually diffuses outwards. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy appears relatively round, with a very slight elongation. Minor disturbances are potentially present in the outer halo, but this is tentative given the image resolution. The color and smooth morphology indicate that the stellar population is likely composed predominantly of older stars, suggesting that the galaxy is likely a red and dead galaxy undergoing little to no star formation.
