The galaxy appears as a single, concentrated object with a generally smooth profile. The core region exhibits a bright, yellowish-white hue, possibly indicating a significant population of older stars. Surrounding the core, there's a more diffuse, bluish halo, which could suggest the presence of younger, hotter stars and some ongoing star formation. The galaxy is primarily round in appearance, with only subtle deviations from a perfect circular shape. No distinct spiral arms or bar structures are discernible. There are no obvious signs of major disturbances or ongoing merger activity. The galaxy seems relatively undisturbed and evolved.
