The observed galaxy presents as a barred spiral structure with a prominent, moderately sized central bulge exhibiting a yellowish hue, potentially indicative of an older stellar population. Spiral arms emerge from the ends of the bar and are wound fairly tightly. These arms show a mottled blue coloration, suggestive of ongoing star formation. The galaxy is well-defined, with a moderately high ellipticity. The spiral arms show a higher luminosity than the space between them and the bulge is brighter than the arms. There is no evidence to suggest that a major merger is occuring, however there is some irregularity visible in the disk that suggests possible minor interactions.
