The galaxy presents as a relatively smooth, disk-shaped structure. It appears to be a spiral galaxy, with a prominent central bulge that has a bright, concentrated core. The disk is tilted with respect to our line of sight, giving it an elongated appearance. There is a hint of spiral arm structure, more apparent on one side, and a general blueness, that suggests ongoing star formation, although it appears subdued. There are some subtle irregularities in the disk, hinting at a possible past interaction. The low presence of prominent distortions suggests a classification of minor disturbance to its structure. The overall light distribution indicates a well-defined object, though not exceptionally luminous at its distance.
