The galaxy presents an overall elliptical morphology, elongated in shape with a smooth, diffuse appearance. The central region exhibits a high concentration of luminosity, appearing significantly brighter than the surrounding areas, indicative of a substantial galactic nucleus. The color profile suggests a population of older stars, with a yellowish hue dominating the galactic body. There is minimal evidence of distinct spiral arm structures or significant dust lanes within the visible spectrum. Faint extensions or tidal features are not readily apparent, implying a relatively undisturbed evolutionary history.
