The galaxy presents as a largely featureless, smooth elliptical or lenticular galaxy. The core is a bright, concentrated yellow, indicating a population of older stars. A slight elongation is observed along one axis, which could be due to rotation, though this is difficult to ascertain without spectroscopic data. There are no apparent spiral arms, dust lanes, or signs of active star formation readily visible in this imaging. The overall color suggests a lack of significant ongoing star formation, indicative of a galaxy dominated by an older stellar population. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or recent mergers.
