This galaxy presents a generally smooth morphology, appearing elliptical in shape rather than displaying spiral arms or a distinct disk structure. Its light profile suggests a centrally concentrated bulge with a gradual decrease in luminosity outward. The galaxy exhibits a color gradient, with a yellowish-white core transitioning to a redder hue in the outer regions. This color distribution implies a population of older, redder stars dominating the outskirts, while the core potentially harbors a mix of stellar populations or ongoing star formation in the green spectrum. There is no apparent evidence of significant dust lanes or tidal features, suggesting a lack of recent major merger events. Minor asymmetry might be present, but is not pronounced.
