The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. A subtle color gradient is observed, transitioning from a slightly bluer hue in the outer regions to a redder tint toward the core, potentially indicating variations in stellar populations or dust distribution. The overall shape appears quite rounded, lacking any obvious signs of significant tidal interactions or major disturbances. There is no indication of prominent spiral arm structures or a well-defined disk component. The galaxy's morphology suggests a system dominated by an older stellar population, consistent with reduced star formation activity.
