This galaxy presents as a spiral galaxy, inclined somewhat to our line of sight. It appears to be dominated by a prominent bulge, which contributes significantly to the overall luminosity. Faint spiral arms can be discerned extending outwards from the central bulge. There are signs of ongoing star formation within the galaxy, with indications of HII regions. A hint of a bar is visible at the center of the galaxy. There is no evidence of any ongoing major merger events.
