The galaxy presents as a moderately elliptical object with a smooth, diffuse light profile, suggesting a substantial spheroidal component. The central region exhibits a bright, concentrated core which may indicate the presence of a supermassive black hole. The major axis is oriented at an angle of approximately 35 degrees relative to the horizontal, with the galaxy appearing slightly elongated. The light distribution suggests a fairly evolved stellar population. There appears to be a slight extension or tidal tail on the right side of the galaxy. The galaxy appears to have a red shift. The data indicates a large galaxy, with a high mass and a moderate amount of star forming.
