The galaxy presents as a disk galaxy, observed at an oblique angle. The bulge appears relatively prominent and centrally concentrated, with a yellow hue, suggesting a population of older stars.  A faint, blueish disk is visible, indicating the presence of younger stars and possibly ongoing star formation. The galaxy appears elongated, with a cigar-like shape. There are no obvious signs of major tidal disturbances or a major merger event. The galaxy appears relatively isolated.
