The galaxy exhibits a spiral structure, with tightly wound arms emanating from a prominent, moderately sized central bulge. The bulge displays a yellowish hue, suggesting an older stellar population. The spiral arms are well-defined, appearing blueish in color. The galaxy appears to be relatively undisturbed with no signs of major mergers or extreme tidal distortions. The dust lanes are well-defined and show a moderate inclination towards our line of sight. The overall shape is somewhat elliptical, suggesting a classification towards the later end of the Hubble sequence.
