The galaxy appears to be a spiral type, exhibiting a relatively face-on orientation. Two prominent spiral arms are visible, emanating from a central bulge. The arms display a somewhat flocculent structure with both medium and loose winding patterns.

The central bulge appears moderately sized, with a yellowish-white color, suggesting an older stellar population. The spiral arms display a bluer hue indicative of ongoing star formation. There's some hint of dust lanes within the spiral arms.

Evidence suggests a possible bar structure, with what appears to be a weak-to-moderate central bar. No significant tidal features or signs of a recent major merger are apparent, though there might be minor disturbances.
