The galaxy presents as a spiral type, exhibiting a prominent disk structure. The spiral arms are well-defined, tracing a relatively grand design. Two spiral arms are clearly visible. The central bulge appears moderately sized, contributing significantly to the overall luminosity of the galaxy. The winding of the spiral arms is intermediate, exhibiting neither a tightly wound nor loosely defined structure. Evidence of a bar feature is apparent, bisecting the central bulge along its major axis. There is no obvious presence of a major ongoing merger event, with the overall structure of the galaxy appearing relatively undisturbed, minor disturbances may be present. The inclination angle to our line of sight suggests the disk is observed at a slight angle. The color profile indicates active star formation regions along the spiral arms, with the central bulge appearing more composed of older stellar populations.
