The galaxy presents an elongated morphology, suggestive of an elliptical or lenticular type. Its light distribution appears relatively smooth and centrally concentrated, with a noticeable color gradient from a bluer periphery towards a redder core. The overall color is skewed toward the redder end of the spectrum. The galaxy exhibits a moderate degree of ellipticity. Evidence for a prominent disk or spiral arm structure is not apparent within the observed image resolution and depth. The galaxy appears relatively isolated, showing no signs of major tidal distortions or ongoing mergers. The galaxy exhibits a redder color than many other galaxies. The galaxy has a red shift that puts it at a considerable distance from our own.