The galaxy presents as a lenticular or edge-on spiral, exhibiting a primarily smooth morphology. The dominant color is a muted blue, suggesting a moderate population of young, hot stars. The galaxy's elongated shape is notable, with a high degree of elongation. There are no visible signs of significant ongoing mergers or major disturbances, although subtle tidal features may be present. The central bulge appears moderately prominent. Overall, the galaxy seems to be a relatively quiescent system, with a low rate of star formation.
