The galaxy presents a largely smooth, elliptical morphology. The light profile exhibits a central concentration, gradually fading outwards. The core appears yellowish-white, suggesting a population of older stars. Surrounding the core, a bluer, less intense halo is visible, possibly indicative of a younger stellar population or some degree of ongoing star formation. There is no readily apparent spiral structure or significant dust lane features. The galaxy shows a slightly rounded shape rather than a highly elongated one. No major signs of interaction, such as tidal tails or highly distorted morphology, are observed, although there might be minor disturbances present in the outer regions. The overall color suggests a system with a substantial mass, placing it within the expected range for elliptical galaxies at a redshift of approximately 0.17.
