The galaxy presents as a single, relatively smooth object with a moderate ellipticity, suggesting an oblate spheroidal shape. The central region exhibits a higher surface brightness, concentrated in a yellowish-white hue that fades gradually into an extended halo. Faint, diffuse extensions are visible on opposing ends along the major axis. There is no apparent structure indicating spiral arms or a well-defined disk, and no obvious signs of recent mergers or major disturbances. The colors appear relatively uniform throughout the galaxy, possibly indicative of an older stellar population.
