The galaxy presents a primarily smooth morphology, exhibiting characteristics of an elliptical galaxy. It appears approximately 7.3 kpc in radius. The central bulge is prominent and displays a concentrated, bright yellowish-orange hue, likely indicative of an older stellar population. There is minimal evidence of significant star formation activity. The overall shape tends towards being in between round and elongated, showing a slight ellipticity rather than a perfectly circular form. There are no visually apparent signs of ongoing or recent major mergers or tidal disturbances; however, faint asymmetry on one side could indicate a minor past interaction.
