The galaxy presents as an elliptical or lenticular type, exhibiting a primarily smooth morphology with a high degree of central concentration. There is a slight asymmetry in the luminosity distribution but no distinct spiral arms. The galaxy appears nearly round, with a hint of elongation but no strong bar feature or significant tidal distortions. The dominant color is in the green, with a small gradient moving toward redder hues in the outer regions. This suggests a relatively older stellar population with less ongoing star formation activity. There appears to be some internal structure visible, but it is not well-defined, indicating it may be a featureless or very old galaxy. There is no evidence of an ongoing major merger, although minor disturbances cannot be ruled out based on the current image resolution.
