This galaxy presents as an elliptical morphology, with a high degree of smoothness. It is slightly elongated. The galaxy exhibits a bright central bulge, which appears to be comprised of older stellar populations given the yellowish color. There is a fainter, diffuse halo of stellar material that extends outwards. There is no clear evidence of spiral arm structure or significant dust lanes. There is no obvious active galactic nucleus activity or indication of a major merger event. There are minor disturbances, but it does not appear to be undergoing a major interaction.
