The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light profile appears to be centrally peaked, with the intensity decreasing gradually outward. The galaxy exhibits a color gradient, with the core appearing more yellow/orange, indicative of an older stellar population dominated by redder stars. The outer regions show a hint of bluer colors, suggesting the presence of a younger stellar population, though less prominent. No obvious spiral arm structures or dust lanes are visible. The galaxy exhibits a somewhat round appearance, with a slight elongation. There are no apparent signs of significant tidal disturbances or ongoing major merger events. The overall structure suggests a relatively evolved system that has largely settled into a stable configuration.
