The galaxy presents as a lenticular or possibly early-type spiral galaxy, exhibiting a relatively smooth light distribution with a high degree of central concentration. A faint disk is suspected, oriented at an oblique angle to the line of sight. The galaxy appears to be undergoing some form of minor disturbance, possibly a small interaction or tidal effect, causing a slight asymmetry in its overall form. The central bulge appears prominent, with an intermediate concentration of stars. The color index suggests the stellar population is old, dominated by low-mass stars, but some star formation is also indicated. There is no strong indication of a recent major merger or violent activity. The object displays an intermediate roundness.
