The galaxy presents as a relatively smooth, cigar-shaped object, likely an elliptical or lenticular galaxy viewed at an oblique angle. There is no readily apparent spiral structure or distinct dust lanes. The galaxy appears to be dominated by older stellar populations, inferred from its yellowish-orange color. There is little evidence of ongoing star formation. The galaxy's shape indicates possible rotational flattening. There may be very minor disturbances visible, but no major merger events or tidal tails are evident in the image. The galaxy appears to be a fairly isolated system.
