The galaxy presents a generally smooth, elliptical morphology. Its shape tends toward being relatively round but not perfectly so. A very small asymmetry could exist, but further investigation would be needed to confirm. The galaxy exhibits a luminosity profile that is brighter and more concentrated toward its center. This implies a higher density of stars or a more active galactic nucleus in that region. The galaxy’s overall color appears moderately red, suggesting an older stellar population and a lower rate of current star formation. There does not appear to be evidence of any ongoing major mergers or significant tidal disturbances.
