The galaxy presents as a grand design spiral with a relatively high degree of rotational symmetry. Two prominent spiral arms are visible, originating from a central bulge. The winding of these arms appears to be of medium tightness. The central bulge constitutes a significant fraction of the galaxy's overall light, with the intensity of light decreasing gradually from the center. The color profile suggests a gradient from a yellowish-orange core to bluer outer arms, which implies differing stellar populations. The redder core may indicate a higher concentration of older stars, while the blue arms could be indicative of ongoing star formation. There appears to be no evidence of significant tidal disturbances or a major merging event. There is no apparent strong bar structure present.
