The galaxy presents as a spiral galaxy, exhibiting a clear disk structure. The spiral arms are well-defined, with a tightly wound morphology and traces of two major arms. Evidence suggests a prominent bar structure bisecting the central bulge. The bulge appears to be of moderate size relative to the overall galactic disk. The galaxy is oriented somewhat face-on, allowing for detailed observation of its spiral structure. Star formation appears to be occurring at a moderate rate. There does not appear to be any major disturbance in the disk. The overall color suggests the galaxy consists of a wide range of stellar populations.
