The galaxy presents as a centrally concentrated, smooth system, most likely an elliptical galaxy. The core is a bright, yellowish-white, suggesting an older stellar population. The light fades in intensity with increasing radial distance from the center. The overall shape appears largely spheroidal, but with a slight elongation. There is very little evidence of spiral arm structure or significant dust lanes. There are no obvious signs of any major tidal disturbances or merging events. The color gradient suggests a centrally concentrated population of older stars, potentially with lower ongoing star formation. The galaxy has a estimated diameter of a few kiloparsecs based on the image scale.
