The galaxy presents as a spiral, with a notable disk. The spiral arms are loosely wound, extending outwards from a bright central bulge. The bulge appears moderately sized in relation to the overall disk. Evidence suggests two dominant spiral arms. The disk exhibits a slight blue hue, potentially indicating ongoing star formation. A faint bar structure may be present within the central region. No significant signs of major merging events are apparent, although minor disturbances cannot be entirely ruled out. The galaxy is not viewed edge-on.
