The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a dominant central bulge that appears smooth and concentrated. The bulge displays a yellowish hue, suggestive of an older stellar population. A faint, flattened disk extends outwards from the bulge and appears elongated. The disk appears to be at an inclined angle relative to our line of sight. There appears to be very little in the way of dust lanes visible, and the disk appears to be relatively uniform in color. One region appears to be a bluer hue relative to the rest of the galaxy, indicating active star formation. Overall the galaxy appears to have a moderate redshift and a low rate of star formation.
