The galaxy presents as a centrally concentrated object, exhibiting a smooth, largely featureless morphology. The light distribution appears radially symmetric, suggesting a classification toward the elliptical end of the Hubble sequence. There is no obvious spiral arm structure, bar, or dust lane visible in this image. The color profile shifts gradually from a yellowish-white core to a bluer halo. This suggests a population of older stars concentrated in the center, surrounded by a population with relatively more younger stars. The overall appearance indicates that this galaxy has likely undergone or is currently undergoing some level of active star formation. There is a possibility of minor disturbances, but it could also be within the realm of observational and image resolution quality.
