The observed galaxy presents as a relatively smooth, elliptical morphology. The galaxy's light profile appears centrally concentrated, with a gradual decrease in intensity outwards. The color index suggests a population of older stars. The presence of some green coloration suggests the possibility of some ongoing, albeit limited, star formation activity. The system does not appear to exhibit significant tidal features or strong asymmetries. Overall, the galaxy appears to be relatively isolated and in a quiescent state. There may be a second galaxy in the lower right. This also appears to be of an eliptical morphology and of similar coloration. More observations are needed to confirm these observations.
