The galaxy presents as a smooth, elliptical-like structure, elongated in shape. It exhibits a concentrated central bulge with a bright, yellowish hue, indicating a population of older stars. The overall light distribution suggests a relatively uniform stellar population, lacking prominent spiral arm structures or distinct star-forming regions. Subtle color gradients may exist, hinting at variations in stellar age or metallicity within the galactic disk. The lack of significant dust lanes or irregular features suggests a dynamically evolved system, possibly nearing the end of its star-forming activity. There appears to be no significant interaction or merging activity occurring, based on the regular and undisturbed structure of the galaxy.
