This galaxy appears to be an elliptical morphology, with a smooth, featureless light distribution. The galaxy's core exhibits a concentrated brightness. The overall color profile suggests a significant population of older stars. There is evidence of a possible recent or ongoing merger event, indicated by the presence of multiple distinct luminous clumps within the galaxy's halo and a tidal tail towards the bottom-right, suggesting a disturbance in the main galaxy's morphology. The galaxy's morphology is largely spheroidal.
