The galaxy appears as a lenticular or early-type spiral galaxy, viewed at a significant angle. Its morphology is somewhat elongated, exhibiting a cigar-like shape. There is evidence of a disk component, although it appears relatively smooth. The galaxy's color profile suggests a moderate presence of older stellar populations, with limited evidence of recent star formation. There may be only minor disturbances that do not appear to be related to a recent or ongoing major merger event.
