The galaxy presents as a spiral type, seen at a slight angle relative to face-on. The central bulge is prominent and appears yellowish, suggesting an older stellar population. The spiral arms are well-defined, displaying a blueish hue indicative of ongoing star formation. There appear to be two relatively distinct spiral arms. These arms seem tightly wound. There is no clear evidence of a bar structure, but a possible weak bar may be present. The disk appears relatively smooth overall, with some signs of flocculent structure within the spiral arms. The galaxy is isolated, showing no signs of major tidal disturbance or ongoing merger activity, though a subtle distortion within the outer disk may indicate minor gravitational interaction.
