The galaxy presents as a spiral type, with a distinct disk structure. The disk is oriented at an angle relative to our line of sight, exhibiting a moderate inclination. Evident spiral arms emanate from the central region, tracing a somewhat grand design morphology. A strong central bar feature bisects the galaxy's core, extending outwards along the major axis. The central bulge is notable, appearing moderate in size relative to the overall galactic structure. There is a general reddish tint and luminosity in the central region. Overall, the spiral arms show intermediate winding with two dominant arms. There does not appear to be signs of major galaxy disruption or merging features.
