The galaxy appears to be a relatively smooth, elliptical system, as it exhibits a largely featureless morphology. Its shape approximates an oblate spheroid, appearing somewhat elongated rather than perfectly circular. There is no obvious spiral arm structure or a well-defined disk component present in the visible light captured in this image. The galaxy's light distribution is concentrated toward the center, and the brightness falls off gradually toward the edges. The galaxy has a blue hue, suggestive of a population of young, hot stars or the presence of ionized gas. It shows minimal evidence of significant tidal disturbances or ongoing major merger activity.
