The galaxy appears to be an elliptical, likely massive system exhibiting a relatively smooth morphology. There is a slight elongation present, although it is predominantly rounded in shape. Light distribution suggests it is generally homogenous, with a slight gradient in color indicative of potential population variations within the galaxy. There are some indications of possible minor tidal disturbance or interaction, but no strong signs of on-going major merging activity. The colors visible suggest it may be dominated by older stellar populations.
