The galaxy appears as an elliptical morphology, with a smooth light distribution and no discernible spiral arm structures. The color suggests that this galaxy likely contains a population of older stars. There is little evidence of significant recent star formation. The estimated size of the galaxy appears to be approximately 10 kpc, making it a relatively average galaxy. The lack of strong color variation indicates a lack of prominent dust lanes. It does not show any visual evidence of ongoing merging activity or major disturbances to its structure. It appears to be a relatively undisturbed galaxy in a quiescent state of evolution.
