The galaxy presents as a generally smooth, centrally concentrated object. It appears elliptical in shape, with a high degree of roundness. The core exhibits a bright, yellowish-white luminosity, suggesting a significant population of older stars. Moving outward from the core, the galaxy displays a gradient shift towards a bluer hue, indicating the presence of a younger stellar population and possible ongoing star formation in the outer regions. There is no apparent spiral structure or significant disk component visible in this image. No signs of major tidal disturbances or interactions with other galaxies are evident, although a very subtle asymmetry may be present in the outer regions. Based on the observed morphology, the galaxy is likely an elliptical galaxy with a moderate mass.
