The galaxy presents as a concentrated, centrally brightened system. Its overall morphology appears smooth and somewhat elliptical, with no prominent spiral arms or bar structure visible in this image. The central region exhibits a yellowish-white hue, which suggests a population of older stars. Fainter, diffuse bluish light extends outwards from the core, possibly indicating the presence of a younger stellar population or ongoing star formation. There is no obvious dust lane or significant morphological disturbance, indicating that the galaxy may be relatively undisturbed and not actively undergoing a major merger. The outer edges of the galaxy fade gradually into the background, with no sharp cutoffs or signs of tidal features.
