The galaxy appears as a centrally concentrated, luminous object with a relatively smooth and round morphology. There is little visible disk-like structure or spiral arm features. Some slight disturbances seem to be present on the outskirts of the galaxy; these could be tidal effects from a possible minor interaction. The galaxy's central region is slightly more concentrated, with the majority of light coming from the galaxy's central region. The red color of the galaxy is indicative of an older stellar population, which suggests a relatively low specific star formation rate. The estimated size of the galaxy is moderate, spanning approximately 6 kiloparsecs in diameter. Overall, the galaxy appears to be a relatively undisturbed, elliptical-like galaxy with an older stellar population and an ongoing, low level of star formation.
