The galaxy presents as an elliptical morphology, characterized by a smooth, featureless light distribution. It has a moderate ellipticity, appearing cigar-shaped, longer than it is wide, but not extremely so. The core of the galaxy displays a slightly reddish hue, indicative of an older stellar population, while the outer regions exhibit a bluer tint, suggesting the presence of some younger, hotter stars. There are no obvious signs of spiral arms, bars, or significant dust lanes. The overall structure appears relatively undisturbed, with no major tidal features or signs of an ongoing merger. The light profile fades gradually from the center outwards, without sharp edges or distinct features.
