The galaxy presents as a somewhat diffuse object with a concentrated central bulge. The light from the galaxy appears yellowish-white, suggesting a population of older stars. There is evidence of disk-like structure or arms but they do not look very well defined. The galaxy exhibits a slightly irregular morphology, hinting at a recent or ongoing interaction or merging event. The luminosity of the object indicates a galaxy of significant size and stellar mass, though the star formation rate seems relatively low. The overall appearance suggests an intermediate stage in its evolution, possibly transitioning from a more actively star-forming spiral to a more quiescent elliptical or lenticular galaxy. There are very subtle features within the disk, it might be a faint ring-like structure, but is difficult to determine due to the resolution.
