The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. The color profile suggests a higher concentration of bluer light in the central region, transitioning to redder hues in the outer regions. The central brightness implies a significant concentration of stellar mass. The overall shape is somewhat elliptical, with a deviation from a perfect circle but it does not appear to be highly elongated or distorted. There is no obvious evidence of spiral arm structure or significant tidal disturbances. The image suggests a relatively quiescent system, consistent with an elliptical galaxy type.
