The galaxy appears as a moderately sized, lenticular or early-type spiral system viewed at a slight angle relative to face-on. Its overall color is suggestive of an older stellar population, with a more prominent concentration of light towards the central bulge. The bulge itself exhibits a smooth morphology, lacking any distinct substructure. There appears to be a faint disk surrounding the bulge. There is no clear evidence of any spiral arm structure in the disk; instead, it seems relatively smooth and featureless. There do not appear to be any significant tidal tails or obvious signs of major mergers or strong interactions with neighboring galaxies. The overall impression is one of relative quiescence.
