The galaxy presents as a somewhat elongated, cigar-shaped structure. A smooth, central bulge dominates its form, exhibiting a yellowish-white hue, indicating an older stellar population. Surrounding the bulge is a fainter, bluer disk component. The blue tint suggests ongoing star formation within this region. The disk appears relatively undisturbed with only some irregularities, suggesting minor disturbances. Overall the galaxy exhibits no strong signs of a recent or ongoing major merger.
