This galaxy presents a generally ordered, disk-like structure. It's orientation is tilted with respect to our line of sight. The galaxy exhibits a bright, concentrated central bulge and notable spiral arms. The arms appear to be tightly wound around the central bulge, implying a relatively high shear rate in the disk. The color of the galaxy suggests a mixed stellar population with regions of both older, redder stars and younger, bluer stars, indicating ongoing star formation. There is a potential for a weak bar structure within the central region. The disk has a smooth appearance, with some signs of minor disturbances, but is mainly without significant major mergers. A faint glow extends beyond the main body of the galaxy.
