This galaxy appears to be a relatively smooth, elliptical system. Its morphology suggests minimal recent merging activity or major disturbances, with a round shape. The galaxy exhibits a bright, concentrated core, and the light gradually diffuses outwards, with no apparent spiral arms or distinct features. There is a slight color gradient observable, with the core appearing bluer compared to the outer regions. This implies the presence of younger, hotter stars in the central region compared to the population in the outskirts. The star formation rate is relatively low. Overall, this galaxy presents as a quiescent system, likely a massive early-type galaxy observed at redshift z≈0.117.
