The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light distribution exhibits a radial gradient, peaking at the core and diminishing outwards. Color indices suggest a population dominated by older stars, with a subtle reddening toward the center. There is no discernible spiral structure or active star-forming regions. Faint extensions or tidal features are absent, indicating a lack of recent major merger events. The galaxy appears relaxed and dynamically evolved.