The galaxy presents as a moderately bright, centrally concentrated object with a roughly elliptical morphology. Its core appears as a bright, unresolved point source indicative of a central bulge, possibly hosting a supermassive black hole. Surrounding the core, there's a diffuse halo of light, fading gradually into the background. The overall color is a faint blue-white, suggesting the presence of a moderate population of young, hot stars, though the lack of distinct spiral arms implies that this galaxy is most likely an early-type spiral or possibly a lenticular galaxy. There are no clear signs of any major disturbances or ongoing mergers. The light distribution is generally smooth, with a high degree of roundness.
