The galaxy presents as a centrally concentrated, largely featureless object. Its light distribution appears smooth and radially symmetric. The color index suggests a population of older stars, as indicated by its redder hue. There is no distinct spiral arm structure or bar visible, suggesting a spheroid-dominated morphology. The absence of significant dust lanes or star-forming regions further supports a relatively quiescent state of star formation. The overall rounded shape indicates a relatively relaxed dynamical state. There is no strong evidence of ongoing mergers or tidal disturbances in this image.
