The galaxy presents as a primarily edge-on disk galaxy. A prominent central bulge is visible, appearing largely spheroidal with a notable degree of roundness. The disk appears smooth, with limited distinct features beyond a general attenuation of light towards the outer edges. There appears to be little to no evidence of significant recent or ongoing merger activity, with no distinct tidal tails or disrupted structures readily apparent. The overall color index suggests a moderate population of older stars. There is no apparent dust lane.
