The galaxy presents as a prominent spiral system, viewed at a relatively high inclination. Two distinct spiral arms are observed, extending outwards from a central bulge. The winding of these arms appears tightly wound. The bulge is moderately sized, with a significant fraction of the galaxy's overall luminosity emanating from this central region. Star formation appears active throughout the galaxy, but is especially concentrated in the spiral arms, as evidenced by their bluer color. The system shows no immediately apparent signs of major mergers or significant tidal disturbances, but minor disturbances may be occurring. The color profile indicates a mature stellar population within the bulge, in contrast to the younger stars populating the spiral arms.
