The galaxy presents as a smooth, elongated structure. It appears elliptical in shape, with a high degree of elongation. The central region exhibits a concentration of light, suggesting a bulge or core. The overall color profile indicates a population of older stars, with a subtle reddish tint throughout the galaxy, but bluer components towards the edges. Faint, diffuse light extends outward from the central region, fading into the background sky. There is no visible spiral structure or dust lanes that can be discerned from this image. The morphology suggests a quiescent galaxy without significant ongoing star formation, but does contain some small signs of star formation. No signs of strong tidal disturbances or mergers are readily apparent, though the image resolution may not allow for identification of subtle interactions.