The observed galaxy presents a flattened, elliptical morphology. A bright, concentrated central bulge is apparent, transitioning smoothly into a less luminous, extended disk. The color gradient suggests a relatively old stellar population, with a yellowish-orange hue dominating the central regions. There are no prominent spiral arms or distinct dust lanes visible, indicating a lack of significant ongoing star formation. The galaxy appears relatively undisturbed, exhibiting no major signs of tidal interactions or recent merger events. Overall, the observed features are consistent with an early-type, disk galaxy nearing quiescence.