The galaxy appears as a slightly elongated spheroid with a smooth, diffuse light distribution. There is no prominent central bulge or spiral arm structure visible at this resolution. The galaxy exhibits a predominantly yellow-orange hue, suggesting a population of older stars and a relatively low rate of on-going star formation. There are no apparent dust lanes or regions of intense blue star formation. The galaxy appears to be relatively isolated, with no immediately obvious signs of tidal interactions or ongoing mergers. The smooth morphology indicates a likelihood that it is an elliptical or lenticular galaxy.
