The galaxy appears as a centrally concentrated object with a relatively smooth overall morphology. The light distribution suggests a dominant bulge component. The color profile appears relatively uniform across the galaxy, with a somewhat yellowish hue, indicating a possible older stellar population. There is no apparent dust lane or prominent spiral arm structure, which is consistent with an early-type or lenticular classification. The overall shape is slightly elliptical, but approaching circular. Based on the red shift, this object is a galaxy billions of light years away. The mass of this object is considerably massive. It appears to not be currently undergoing a major merging event, as there are no tidal tails visible.
