The observed galaxy presents as a spiral galaxy, exhibiting a disk-like structure viewed at a slight angle to our line of sight. The galaxy possesses a moderately sized central bulge, appearing as a concentrated region of light. Evident spiral arms emanate from this central region, displaying a tightly wound morphology, with at least three arms being visible. The arms contain areas that suggest active star formation. The lack of an obvious bar structure is noted. Minor disturbances in the disk do not appear to be occurring.
